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	<title>A0535+26 - Revision history</title>
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	<updated>2026-05-30T22:29:19Z</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=A0535%2B26&amp;diff=1237&amp;oldid=prev</id>
		<title>Kuehnel: Created page with &quot;Category:Accreting X-ray Pulsars   '''This page is still edited'''   = System Overview =  {| class=&quot;wikitable&quot; |P&lt;sub&gt;orb&lt;/sub&gt;  | 111.1  | days  | Finger et al. 2006  |-...&quot;</title>
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		<updated>2018-04-18T12:20:36Z</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;   &amp;#039;&amp;#039;&amp;#039;This page is still edited&amp;#039;&amp;#039;&amp;#039;   = System Overview =  {| class=&amp;quot;wikitable&amp;quot; |P&amp;lt;sub&amp;gt;orb&amp;lt;/sub&amp;gt;  | 111.1  | days  | Finger et al. 2006  |-...&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;
&lt;br /&gt;
'''This page is still edited'''&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
= System Overview =&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|P&amp;lt;sub&amp;gt;orb&amp;lt;/sub&amp;gt; &lt;br /&gt;
| 111.1 &lt;br /&gt;
| days &lt;br /&gt;
| Finger et al. 2006 &lt;br /&gt;
|- &lt;br /&gt;
|P&amp;lt;sub&amp;gt;spin&amp;lt;/sub&amp;gt; &lt;br /&gt;
| 103.4 &lt;br /&gt;
| s &lt;br /&gt;
| Rosenberg et al. 1975, Makino et al. 1989, ... &lt;br /&gt;
|- &lt;br /&gt;
|B &lt;br /&gt;
| 4x10&amp;lt;sup&amp;gt;12&amp;lt;/sup&amp;gt; &lt;br /&gt;
| G &lt;br /&gt;
| Kendziorra et al. 1994 &lt;br /&gt;
|- &lt;br /&gt;
|a sin i &lt;br /&gt;
| 267 &lt;br /&gt;
| lt-sec &lt;br /&gt;
| Finger et al. 2006 &lt;br /&gt;
|- &lt;br /&gt;
|eccentricity &lt;br /&gt;
| 0.47 &lt;br /&gt;
| &lt;br /&gt;
| Finger et al. 2006 &lt;br /&gt;
|- &lt;br /&gt;
|ω &lt;br /&gt;
| 130 &lt;br /&gt;
|degree &lt;br /&gt;
| Finger et al. 2006 &lt;br /&gt;
|- &lt;br /&gt;
|Τ&amp;lt;sub&amp;gt;periastron&amp;lt;/sub&amp;gt; &lt;br /&gt;
| 53613.0 &lt;br /&gt;
| MJD &lt;br /&gt;
| Finger et al. 2006 &lt;br /&gt;
|- &lt;br /&gt;
|distance &lt;br /&gt;
| 2 &lt;br /&gt;
| kpc &lt;br /&gt;
| Steele et al. 1994 &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
= Optical companion =&lt;br /&gt;
&lt;br /&gt;
HDE 245770, spectral class: O9.7IIIe (Giangrande et al. 1980), B0 IIIe (Steele et al. 1998) &amp;lt;br /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|M &lt;br /&gt;
| 14 / 20 / 26 &lt;br /&gt;
| M&amp;lt;sub&amp;gt;⊙&amp;lt;/sub&amp;gt; &lt;br /&gt;
| de Loore et al. 1984 / Coe et al. 2006 / Haigh et al. 2004 &lt;br /&gt;
|- &lt;br /&gt;
|R &lt;br /&gt;
| 14 &lt;br /&gt;
| R&amp;lt;sub&amp;gt;⊙&amp;lt;/sub&amp;gt; &lt;br /&gt;
|de Loore et al. 1984 &lt;br /&gt;
|- &lt;br /&gt;
|Mdot &lt;br /&gt;
| 10&amp;lt;sup&amp;gt;-8&amp;lt;/sup&amp;gt; &lt;br /&gt;
| M&amp;lt;sub&amp;gt;⊙&amp;lt;/sub&amp;gt; &lt;br /&gt;
|de Loore et al. 1984 &lt;br /&gt;
|- &lt;br /&gt;
|T&amp;lt;sub&amp;gt;eff&amp;lt;/sub&amp;gt; &lt;br /&gt;
| 26000-28000 &lt;br /&gt;
| K &lt;br /&gt;
| Giovannelli &amp;amp; Graziati 1992 &lt;br /&gt;
|- &lt;br /&gt;
|L &lt;br /&gt;
| 0.7 x 10&amp;lt;sup&amp;gt;5&amp;lt;/sup&amp;gt; &lt;br /&gt;
| L&amp;lt;sub&amp;gt;⊙&amp;lt;/sub&amp;gt; &lt;br /&gt;
| Giovannelli &amp;amp; Graziati 1992 &lt;br /&gt;
|}&lt;br /&gt;
= Description =&lt;br /&gt;
&lt;br /&gt;
=== Pulse period and pulse profiles ===&lt;br /&gt;
&lt;br /&gt;
* pulse shape and intensity are highly variable (Frontera et al. 1985) &lt;br /&gt;
* lower energies several, irregularly spaced maxima observed (bradt et al. 1976)&lt;br /&gt;
* double-peaked pulse profiles above 20 keV&lt;br /&gt;
* asymmetric main and more symmetric secondary peak (Kendziorra et al. 1994)&lt;br /&gt;
* pulsed fraction increases with energy (Frontera et al. 1985, Kendziorra et al. 1994)&lt;br /&gt;
&lt;br /&gt;
=== Spectrum ===&lt;br /&gt;
&lt;br /&gt;
* hard power law with index 0.8-1.1 with exponential cutoff (Ricketts et al. 1975, Kendziorra et al. 1994) &lt;br /&gt;
* 2 cyclotron lines at about 50, 100 keV&lt;br /&gt;
* Pulse phase analysis: main pulse spectrum harder than secondary pulse (Kendziorra et al. 1994)&lt;/div&gt;</summary>
		<author><name>Kuehnel</name></author>
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