https://www.sternwarte.uni-erlangen.de/wiki/index.php?action=history&feed=atom&title=Head16 2026-05-27T06:08:12Z Revision history for this page on the wiki MediaWiki 1.35.7 https://www.sternwarte.uni-erlangen.de/wiki/index.php?title=Head16&diff=1608&oldid=prev 2018-06-25T13:31:49Z

<p>Fixed links to PDF files</p> <table class="diff diff-contentalign-left diff-editfont-monospace" data-mw="interface"> <col class="diff-marker" /> <col class="diff-content" /> <col class="diff-marker" /> <col class="diff-content" /> <tr class="diff-title" lang="en"> <td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">← Older revision</td> <td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">Revision as of 13:31, 25 June 2018</td> </tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l24" >Line 24:</td> <td colspan="2" class="diff-lineno">Line 24:</td></tr> <tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==== Related Poster Presentations ====</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==== Related Poster Presentations ====</div></td></tr> <tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr> <tr><td class='diff-marker'>−</td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>   * 120.03: <del class="diffchange diffchange-inline">{{:head16</del>:poster_bodaghee_small.pdf|NuSTAR discovers a cyclotron line and reveals the spinning up of the accreting X-ray pulsar IGR J16393-4643<del class="diffchange diffchange-inline">}}</del>\\ Arash Bodaghee (Georgia College)</div></td><td class='diff-marker'>+</td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>   * 120.03: <ins class="diffchange diffchange-inline">[[Media</ins>:poster_bodaghee_small.pdf|NuSTAR discovers a cyclotron line and reveals the spinning up of the accreting X-ray pulsar IGR J16393-4643<ins class="diffchange diffchange-inline">]]</ins>\\ Arash Bodaghee (Georgia College)</div></td></tr> <tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr> <tr><td class='diff-marker'>−</td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>   * 120.06: <del class="diffchange diffchange-inline">{{:head16</del>:brumbackheadposter.pdf|An investigation of luminous X-ray pulsars: Exploring accretion onto the magnetized neutron star LMC X-4<del class="diffchange diffchange-inline">}}</del>\\ McKinley C. Brumback (Dartmouth College)</div></td><td class='diff-marker'>+</td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>   * 120.06: <ins class="diffchange diffchange-inline">[[Media</ins>:brumbackheadposter.pdf|An investigation of luminous X-ray pulsars: Exploring accretion onto the magnetized neutron star LMC X-4<ins class="diffchange diffchange-inline">]]</ins>\\ McKinley C. Brumback (Dartmouth College)</div></td></tr> <tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr> <tr><td class='diff-marker'>−</td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>   * 120.09: <del class="diffchange diffchange-inline">{{:head16</del>:cenx3b.pdf|The broadband spectrum of Centaurus X-3<del class="diffchange diffchange-inline">}}</del>\\ Amy M. Gottlieb (Univ. Florida &amp; UMBC &amp; NASA-GSFC)</div></td><td class='diff-marker'>+</td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>   * 120.09: <ins class="diffchange diffchange-inline">[[Media</ins>:cenx3b.pdf|The broadband spectrum of Centaurus X-3<ins class="diffchange diffchange-inline">]]</ins>\\ Amy M. Gottlieb (Univ. Florida &amp; UMBC &amp; NASA-GSFC)</div></td></tr> <tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr> <tr><td class='diff-marker'>−</td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>   * 120.21: <del class="diffchange diffchange-inline">{{:head16</del>:gx304_poster3.pdf|Discovery and model of a rollover in the positive cyclotron line / luminosity relation in GX 304-1 with RXTE<del class="diffchange diffchange-inline">}}</del>\\ Richard E. Rothschild (CASS-UCSD)</div></td><td class='diff-marker'>+</td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>   * 120.21: <ins class="diffchange diffchange-inline">[[Media</ins>:gx304_poster3.pdf|Discovery and model of a rollover in the positive cyclotron line / luminosity relation in GX 304-1 with RXTE<ins class="diffchange diffchange-inline">]]</ins>\\ Richard E. Rothschild (CASS-UCSD)</div></td></tr> <tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr> <tr><td class='diff-marker'>−</td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>   * 120:24: <del class="diffchange diffchange-inline">{{:head16</del>:head.herx1.poster.v2.mar312016.pdf|The NuSTAR X-ray Spectrum of Hercules X-1: A radiation-dominated radiative shock<del class="diffchange diffchange-inline">}}</del>\\ Michael T. Wolff (NRL)</div></td><td class='diff-marker'>+</td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>   * 120:24: <ins class="diffchange diffchange-inline">[[Media</ins>:head.herx1.poster.v2.mar312016.pdf|The NuSTAR X-ray Spectrum of Hercules X-1: A radiation-dominated radiative shock<ins class="diffchange diffchange-inline">]]</ins>\\ Michael T. Wolff (NRL)</div></td></tr> </table>

Thalhammer https://www.sternwarte.uni-erlangen.de/wiki/index.php?title=Head16&diff=1607&oldid=prev 2018-06-25T13:30:30Z

<p>Fixed links to PDF files</p> <table class="diff diff-contentalign-left diff-editfont-monospace" data-mw="interface"> <col class="diff-marker" /> <col class="diff-content" /> <col class="diff-marker" /> <col class="diff-content" /> <tr class="diff-title" lang="en"> <td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">← Older revision</td> <td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">Revision as of 13:30, 25 June 2018</td> </tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l6" >Line 6:</td> <td colspan="2" class="diff-lineno">Line 6:</td></tr> <tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==== HEAD Meeting 2016 Special Session 201, Talks ====</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==== HEAD Meeting 2016 Special Session 201, Talks ====</div></td></tr> <tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr> <tr><td class='diff-marker'>−</td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>   <del class="diffchange diffchange-inline">* </del>201.01: <del class="diffchange diffchange-inline">{{:head16</del>:head.mtw.overview.july252016.website_small.pdf|Accretion Powered X-ray pulsars: Physics of the accretion column<del class="diffchange diffchange-inline">}}</del>\\ Michael T. Wolff (NRL)</div></td><td class='diff-marker'>+</td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>   201.01: <ins class="diffchange diffchange-inline">[[Media</ins>:head.mtw.overview.july252016.website_small.pdf|Accretion Powered X-ray pulsars: Physics of the accretion column<ins class="diffchange diffchange-inline">]]</ins>\\ Michael T. Wolff (NRL)</div></td></tr> <tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr> <tr><td class='diff-marker'>−</td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>   * 201.02: <del class="diffchange diffchange-inline">{{:head16</del>:dianacheatham_head_2016_presentation.pdf|Application of a physical continuum model to recent X-ray observations of accreting pulsars<del class="diffchange diffchange-inline">}}</del>\\ Diana M. Marcu-Cheatham (UMBC &amp; NASA-GSFC)</div></td><td class='diff-marker'>+</td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>   * 201.02: <ins class="diffchange diffchange-inline">[[Media</ins>:dianacheatham_head_2016_presentation.pdf|Application of a physical continuum model to recent X-ray observations of accreting pulsars<ins class="diffchange diffchange-inline">]]</ins>\\ Diana M. Marcu-Cheatham (UMBC &amp; NASA-GSFC)</div></td></tr> <tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr> <tr><td class='diff-marker'>−</td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>   * 201.03: <del class="diffchange diffchange-inline">{{:head16</del>:crsf.pdf|Cyclotron lines<del class="diffchange diffchange-inline">}}</del>\\ Jörn Wilms (Remeis Observatory, FAU)</div></td><td class='diff-marker'>+</td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>   * 201.03: <ins class="diffchange diffchange-inline">[[Media</ins>:crsf.pdf|Cyclotron lines<ins class="diffchange diffchange-inline">]]</ins>\\ Jörn Wilms (Remeis Observatory, FAU)</div></td></tr> <tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr> <tr><td class='diff-marker'>−</td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>   * 201.04: <del class="diffchange diffchange-inline">{{:head16</del>:spelum.pdf|Spectrum-luminosity dependence of radiation from polar emitting regions in accreting magnetized neutron stars<del class="diffchange diffchange-inline">}}</del>\\ Dmitry Klochkov (IAA Tübingen)</div></td><td class='diff-marker'>+</td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>   * 201.04: <ins class="diffchange diffchange-inline">[[Media</ins>:spelum.pdf|Spectrum-luminosity dependence of radiation from polar emitting regions in accreting magnetized neutron stars<ins class="diffchange diffchange-inline">]]</ins>\\ Dmitry Klochkov (IAA Tübingen)</div></td></tr> <tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr> <tr><td class='diff-marker'>−</td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>   * 201.05: <del class="diffchange diffchange-inline">{{:head16</del>:201.05_staubert.pdf|Long-term change in the cyclotron line energy in Hercules X-1<del class="diffchange diffchange-inline">}}</del>\\ Rüdiger Staubert (IAA Tübingen)</div></td><td class='diff-marker'>+</td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>   * 201.05: <ins class="diffchange diffchange-inline">[[Media</ins>:201.05_staubert.pdf|Long-term change in the cyclotron line energy in Hercules X-1<ins class="diffchange diffchange-inline">]]</ins>\\ Rüdiger Staubert (IAA Tübingen)</div></td></tr> <tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr> <tr><td class='diff-marker'>−</td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>   * 201.06: <del class="diffchange diffchange-inline">{{:head16</del>:hemphill_head2016_talk.pdf|Evidence for an evolving cyclotron line energy in 4U 1538-522<del class="diffchange diffchange-inline">}}</del>\\ Paul B. Hemphill (CASS-UCSD)</div></td><td class='diff-marker'>+</td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>   * 201.06: <ins class="diffchange diffchange-inline">[[Media</ins>:hemphill_head2016_talk.pdf|Evidence for an evolving cyclotron line energy in 4U 1538-522<ins class="diffchange diffchange-inline">]]</ins>\\ Paul B. Hemphill (CASS-UCSD)</div></td></tr> <tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr> <tr><td class='diff-marker'>−</td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>   * 201.07: <del class="diffchange diffchange-inline">{{:head16</del>:head_naples_nustar_pulsars.pdf|Pulsar observations with NuSTAR<del class="diffchange diffchange-inline">}}</del>\\ Felix Fürst (Caltech)</div></td><td class='diff-marker'>+</td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>   * 201.07: <ins class="diffchange diffchange-inline">[[Media</ins>:head_naples_nustar_pulsars.pdf|Pulsar observations with NuSTAR<ins class="diffchange diffchange-inline">]]</ins>\\ Felix Fürst (Caltech)</div></td></tr> <tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr> <tr><td class='diff-marker'>−</td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>   * 201.08: <del class="diffchange diffchange-inline">{{:head16</del>:201604_head.pdf|Self-consistent accretion column modeling<del class="diffchange diffchange-inline">}}</del>\\ Sebastian Falkner (Remeis Observatory, FAU)</div></td><td class='diff-marker'>+</td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>   * 201.08: <ins class="diffchange diffchange-inline">[[Media</ins>:201604_head.pdf|Self-consistent accretion column modeling<ins class="diffchange diffchange-inline">]]</ins>\\ Sebastian Falkner (Remeis Observatory, FAU)</div></td></tr> <tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr> <tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==== Related Poster Presentations ====</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==== Related Poster Presentations ====</div></td></tr> </table>

Thalhammer https://www.sternwarte.uni-erlangen.de/wiki/index.php?title=Head16&diff=1470&oldid=prev 2018-05-03T08:08:20Z

<p>Created page with &quot; <a href="/wiki/index.php/Category:Accreting_X-ray_Pulsars" title="Category:Accreting X-ray Pulsars">Category:Accreting X-ray Pulsars</a> ==== HEAD Meeting 2016 Special Session 201, Talks ==== * 201.01: {{:head16:head.mtw.overview.july252016.website_small.pdf|Accretion...&quot;</p> <p><b>New page</b></p><div><br /> <br /> [[Category:Accreting X-ray Pulsars]]<br /> <br /> <br /> ==== HEAD Meeting 2016 Special Session 201, Talks ====<br /> <br /> * 201.01: {{:head16:head.mtw.overview.july252016.website_small.pdf|Accretion Powered X-ray pulsars: Physics of the accretion column}}\\ Michael T. Wolff (NRL)<br /> <br /> * 201.02: {{:head16:dianacheatham_head_2016_presentation.pdf|Application of a physical continuum model to recent X-ray observations of accreting pulsars}}\\ Diana M. Marcu-Cheatham (UMBC &amp; NASA-GSFC)<br /> <br /> * 201.03: {{:head16:crsf.pdf|Cyclotron lines}}\\ Jörn Wilms (Remeis Observatory, FAU)<br /> <br /> * 201.04: {{:head16:spelum.pdf|Spectrum-luminosity dependence of radiation from polar emitting regions in accreting magnetized neutron stars}}\\ Dmitry Klochkov (IAA Tübingen)<br /> <br /> * 201.05: {{:head16:201.05_staubert.pdf|Long-term change in the cyclotron line energy in Hercules X-1}}\\ Rüdiger Staubert (IAA Tübingen)<br /> <br /> * 201.06: {{:head16:hemphill_head2016_talk.pdf|Evidence for an evolving cyclotron line energy in 4U 1538-522}}\\ Paul B. Hemphill (CASS-UCSD)<br /> <br /> * 201.07: {{:head16:head_naples_nustar_pulsars.pdf|Pulsar observations with NuSTAR}}\\ Felix Fürst (Caltech)<br /> <br /> * 201.08: {{:head16:201604_head.pdf|Self-consistent accretion column modeling}}\\ Sebastian Falkner (Remeis Observatory, FAU)<br /> <br /> ==== Related Poster Presentations ====<br /> <br /> * 120.03: {{:head16:poster_bodaghee_small.pdf|NuSTAR discovers a cyclotron line and reveals the spinning up of the accreting X-ray pulsar IGR J16393-4643}}\\ Arash Bodaghee (Georgia College)<br /> <br /> * 120.06: {{:head16:brumbackheadposter.pdf|An investigation of luminous X-ray pulsars: Exploring accretion onto the magnetized neutron star LMC X-4}}\\ McKinley C. Brumback (Dartmouth College)<br /> <br /> * 120.09: {{:head16:cenx3b.pdf|The broadband spectrum of Centaurus X-3}}\\ Amy M. Gottlieb (Univ. Florida &amp; UMBC &amp; NASA-GSFC)<br /> <br /> * 120.21: {{:head16:gx304_poster3.pdf|Discovery and model of a rollover in the positive cyclotron line / luminosity relation in GX 304-1 with RXTE}}\\ Richard E. Rothschild (CASS-UCSD)<br /> <br /> * 120:24: {{:head16:head.herx1.poster.v2.mar312016.pdf|The NuSTAR X-ray Spectrum of Hercules X-1: A radiation-dominated radiative shock}}\\ Michael T. Wolff (NRL)</div>

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