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	<id>https://www.sternwarte.uni-erlangen.de/wiki/index.php?action=history&amp;feed=atom&amp;title=MXB_0656-07</id>
	<title>MXB 0656-07 - Revision history</title>
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	<updated>2026-05-30T10:31:18Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
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		<id>https://www.sternwarte.uni-erlangen.de/wiki/index.php?title=MXB_0656-07&amp;diff=1238&amp;oldid=prev</id>
		<title>Kuehnel: Created page with &quot;Category:Accreting X-ray Pulsars  [http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=+MXB+0656-072&amp;submit=SIMBAD+search simbad]  Transient source, discovered in 1975 by SA...&quot;</title>
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		<updated>2018-04-18T12:23:40Z</updated>

		<summary type="html">&lt;p&gt;Created page with &amp;quot;&lt;a href=&quot;/wiki/index.php/Category:Accreting_X-ray_Pulsars&quot; title=&quot;Category:Accreting X-ray Pulsars&quot;&gt;Category:Accreting X-ray Pulsars&lt;/a&gt;  [http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=+MXB+0656-072&amp;amp;submit=SIMBAD+search simbad]  Transient source, discovered in 1975 by SA...&amp;quot;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;[[Category:Accreting X-ray Pulsars]]&lt;br /&gt;
&lt;br /&gt;
[http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=+MXB+0656-072&amp;amp;submit=SIMBAD+search simbad]&lt;br /&gt;
&lt;br /&gt;
Transient source, discovered in 1975 by SAS-3 (&amp;lt;ref name=&amp;quot;Clark75&amp;quot; /&amp;gt;).&lt;br /&gt;
&lt;br /&gt;
In quiescence since 1975/1976, it became active again in 2003 with an outburst in October 2003  (&amp;lt;ref name=&amp;quot;Remillard03&amp;quot; /&amp;gt;).&lt;br /&gt;
&lt;br /&gt;
New outburst detected in November 2007 (&amp;lt;ref name=&amp;quot;Kreykenbohm07&amp;quot; /&amp;gt;). &lt;br /&gt;
&lt;br /&gt;
Monitoring data: [http://xte.mit.edu/XTE/asmlc/srcs/x0656-072.html  RXTE/ASM], &lt;br /&gt;
[http://swift.gsfc.nasa.gov/docs/swift/results/transients/weak/MXB0656-072/ Swift/BAT], &lt;br /&gt;
[http://maxi.riken.jp/top/index.php?cid=1&amp;amp;jname=J0658-072  MAXI], &lt;br /&gt;
[http://www.batse.msfc.nasa.gov/gbm/science/pulsars/lightcurves/mxb0656.html Fermi/GBM ]&lt;br /&gt;
&lt;br /&gt;
= Coordinates = &lt;br /&gt;
&lt;br /&gt;
RA 06h 58m 16.80s,    DEC -07° 12' 37.8'' (J2000)&amp;lt;br /&amp;gt;&lt;br /&gt;
l 220.1283°, b -01.7694° (J2000)&lt;br /&gt;
&lt;br /&gt;
= Optical companion = &lt;br /&gt;
&lt;br /&gt;
O9.7Ve ([(biblio:Pakull03)]).&lt;br /&gt;
&lt;br /&gt;
= Binary system =&lt;br /&gt;
&lt;br /&gt;
Distance: 3.9 +/-0.1 kpc &amp;lt;ref name=&amp;quot;McBride06&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
= Orbit =&lt;br /&gt;
&lt;br /&gt;
The orbital period of the system was determined to '''101.2 d''' using the outburst spacing seen in RXTE/ASM and Swift/BAT (&amp;lt;ref name=&amp;quot;Yan2012&amp;quot; /&amp;gt;). The remaining orbital parameters of the system remain undetermined.&lt;br /&gt;
= Spectrum =&lt;br /&gt;
&lt;br /&gt;
Continuum spectrum well described with a power law with an exponential cutoff. &lt;br /&gt;
&lt;br /&gt;
Cyclotron line at ~35 keV discovered by &amp;lt;ref name=&amp;quot;Heindl03b&amp;quot; /&amp;gt; with RXTE. &lt;br /&gt;
&lt;br /&gt;
Study of the cyclotron line with RXTE in &amp;lt;ref name=&amp;quot;McBride06&amp;quot; /&amp;gt;. &lt;br /&gt;
&lt;br /&gt;
= Pulse period =&lt;br /&gt;
&lt;br /&gt;
Average pulse period of 160.4+/-0.4 s, spin-up Pdot=-0.0202+/-0.0003 s/day during the 2003 outburst. &lt;br /&gt;
&lt;br /&gt;
Pulse period monitored with [http://www.batse.msfc.nasa.gov/gbm/science/pulsars/lightcurves/mxb0656.html Fermi/GBM ]&lt;br /&gt;
&lt;br /&gt;
= Pulse profiles =&lt;br /&gt;
&lt;br /&gt;
Single-peaked and sinusoidal in all energy ranges (2-60 keV). &lt;br /&gt;
&lt;br /&gt;
Pulsed fraction (Fmax-Fmin/Fmax) increases steadily from 26% in the 2-5 keV band up to 40% in the 30-60 keV band &amp;lt;ref name=&amp;quot;McBride06&amp;quot; /&amp;gt;. &lt;br /&gt;
&lt;br /&gt;
'''References'''&lt;/div&gt;</summary>
		<author><name>Kuehnel</name></author>
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