Erdeve, Işıl and Kalemci, Emrah and Alpar, M. Ali (2009) Hard X-Ray flux upper limits of central compact objects in supernova remnants. The Astrophysical Journal, 696 (2). pp. 1792-1797. ISSN 0004-637X
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Official URL: http://dx.doi.org/10.1088/0004-637X/696/2/1792
Abstract
We searched for hard X-ray (20–300 keV) emission from nine central compact
objects (CCOs) 1E 1207.4−5209, 1WGA J1713−3949, J082157.5−430017,
J085201.4−461753, J1601−5133, J1613483−5055, J181852.0−150213,
J185238.6+004020, and J232327.9+584843 with the INTEGRAL observatory.
We applied spectral imaging analysis and did not detect any of the sources
with luminosity upper limits in the range of 1033-1034 ergs/s in the 20-75 keV
band. For nearby CCOs (< 4 kpc) the upper limit luminosities are an order
of magnitude lower than the measured persistent hard X-ray luminosities of
AXPs. This may indicate that the central compact objects are low magnetic
field systems with fallback disks around them.
Item Type: | Article |
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Uncontrolled Keywords: | stars: neutron; supernova remnants; X-rays: stars |
Subjects: | Q Science > QB Astronomy > QB460-466 Astrophysics Q Science > QC Physics > QC1 General |
Divisions: | Faculty of Engineering and Natural Sciences > Basic Sciences > Physics |
Depositing User: | Emrah Kalemci |
Date Deposited: | 08 Sep 2009 09:55 |
Last Modified: | 23 Jul 2019 09:57 |
URI: | https://research.sabanciuniv.edu/id/eprint/11880 |
Available Versions of this Item
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Hard X-Ray flux upper limits of central compact objects in
supernova remnants. (deposited 22 Oct 2008 17:07)
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Hard X-Ray flux upper limits of central compact objects in
supernova remnants. (deposited 02 Mar 2009 16:08)
- Hard X-Ray flux upper limits of central compact objects in supernova remnants. (deposited 08 Sep 2009 09:55) [Currently Displayed]
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Hard X-Ray flux upper limits of central compact objects in
supernova remnants. (deposited 02 Mar 2009 16:08)