scholarly journals Near‐Infrared and Optical Limits for the Central X‐Ray Point Source in the Cassiopeia A Supernova Remnant

2006 ◽  
Vol 636 (2) ◽  
pp. 848-858 ◽  
Author(s):  
R. A. Fesen ◽  
G. G. Pavlov ◽  
D. Sanwal
2001 ◽  
Vol 558 (1) ◽  
pp. 270-275 ◽  
Author(s):  
D. L. Kaplan ◽  
S. R. Kulkarni ◽  
S. S. Murray

1975 ◽  
Vol 200 ◽  
pp. 158 ◽  
Author(s):  
R. W. Hill ◽  
G. A. Burginyon ◽  
F. D. Seward
Keyword(s):  
X Ray ◽  

1980 ◽  
Vol 193 (2) ◽  
pp. 175-188 ◽  
Author(s):  
A. C. Fabian ◽  
R. Willingale ◽  
J. P. Pye ◽  
S. S. Murray ◽  
G. Fabbiano
Keyword(s):  
X Ray ◽  

2014 ◽  
pp. 15-24 ◽  
Author(s):  
T.J. Galvin ◽  
M.D. Filipovic

We present Data Release 2 of the Point Source Catalogue created from a series of previously constructed radio-continuum images of M31 at ?=20 cm (v=1.4 GHz) from archived VLA observations. In total, we identify a collection of 916 unique discrete radio sources across the field of M31. Comparing these detected sources to those listed by Gelfand et al. (2004) at ?=92 cm, the spectral index of 98 sources has been derived. The majority (73%) of these sources exhibit a spectral index of ?<-0.6, indicating that their emission is predominantly non-thermal in nature, which is typical for background objects and Supernova Remnants (SNRs). Additionally, we investigate the presence of radio counterparts for some 156 SNRs and SNR candidates, finding a total of only 13 of these objects in our images within a 500 search area. Auxiliary optical, radio and X-ray catalogues were cross referenced highlighting a small population of SNRs and SNR candidates common to multi frequency domains.


2020 ◽  
Vol 896 (2) ◽  
pp. 177
Author(s):  
Bon-Chul Koo ◽  
Hyun-Jeong Kim ◽  
Yong-Hyun Lee ◽  
John C. Raymond ◽  
Jae-Joon Lee ◽  
...  

1998 ◽  
Vol 505 (1) ◽  
pp. L27-L30 ◽  
Author(s):  
Barron Koralesky ◽  
L. Rudnick ◽  
E. V Gotthelf ◽  
J. W. Keohane
Keyword(s):  
X Ray ◽  

2017 ◽  
Vol 836 (2) ◽  
pp. 225 ◽  
Author(s):  
Toshiki Sato ◽  
Yoshitomo Maeda ◽  
Aya Bamba ◽  
Satoru Katsuda ◽  
Yutaka Ohira ◽  
...  

2013 ◽  
Vol 9 (S296) ◽  
pp. 380-381
Author(s):  
Lab Saha ◽  
Tulun Ergin ◽  
Pratik Majumdar ◽  
Mustafa Bozkurt

AbstractWe have analyzed Chandra X-ray data from different parts of the shell of young supernova remnant (SNR) in the energy range of 0.7 - 8 keV. We observed that X-ray flux level varies over different shell regions of the source. Implications of X-ray observation will be discussed here. We also analyzed Fermi-LAT data in the energy range 0.5 - 50 GeV for the source. The differential spectrum obtained in this way fits with simple power-law. We also present here multi-wavelength modeling of the source considering archival radio and TeV data along with Chandra and Fermi-LAT data.


Supernova remnants are now recognized as a class of soft X-ray emitting-objects. The evolution of a remnant’s X-ray emission is discussed and a number of possible X-ray emission mechanisms are described. The spectrum of the Crab Nebula has been studied with Copernicus. The data have been used to derive a value of the gas column density of the interstellar medium. The X-ray structure and spectrum of the remnant Cassiopeia. A have been investigated and the results are presented. A high resolution X-ray map of the Puppis A supernova remnant has been obtained and the interpretation of the X-ray structure is discussed. X-ray emission has been detected from the pulsar PSR 08 33-45. This observation is compared with data obtained from the Uhuru satellite in order to derive the gas column density to the source. Weak soft X-ray emission has been detected from the Cygnus Loop in the regions expected but a t a lower intensity – a search for regions of higher intensity is continuing. A programme to identify known radio remnants as X-ray emitters is in progress and the results obtained so far are reported.


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