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相关论文: X-ray supernova remnants in nearby galaxies

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We present results from a study of the Supernova Remnant (SNR) population in a sample of six nearby galaxies (NGC 2403, NGC 3077, NGC 4214, NGC 4449, NGC 4395 and NGC 5204) based on Chandra archival data. We have detected 244 discrete X-ray…

高能天体物理现象 · 物理学 2015-05-19 Ioanna Leonidaki , Andreas Zezas , Panayotis Boumis

We present results from a study of optically emitting Supernova Remnants (SNRs) in six nearby galaxies (NGC 2403, NGC 3077, NGC 4214, NGC 4395, NGC 4449 and NGC 5204) based on deep narrow band H{\alpha} and [SII] images as well as…

宇宙学与河外天体物理 · 物理学 2015-06-12 I. Leonidaki , P. Boumis , A. Zezas

This work focuses on the detection of X-ray Supernova Remnants (SNRs) in the galaxy NGC 7793 and the study of their properties. X-ray SNRs in galaxies beyond the Local Group are rare, mainly due to the limited sensitivity of current X-ray…

高能天体物理现象 · 物理学 2025-09-10 Maria Kopsacheili , Konstantina Anastasopoulou , Nanda Rea , Claudia Patricia Gutiérrez , Lluís Galbany

We present the analysis of supernova remnants (SNRs) and candidates in M31 identified in the XMM-Newton large programme survey of M31. SNRs are among the bright X-ray sources in a galaxy. They are good indicators of recent star formation…

We present the second in a series of results in which we have searched for undiscovered neutron stars in supernova remnants (SNRs). This paper deals with the largest six SNRs in our sample, too large for Chandra or XMM-Newton to cover in a…

天体物理学 · 物理学 2009-11-11 D. L. Kaplan , B. M. Gaensler , S. R. Kulkarni , P. O. Slane

Using a combination of ground-based and HST imaging, we have constructed a catalog of 179 supernova remnants (SNRs) and SNR candidates in the nearby spiral galaxy M51. Follow-up spectroscopy of 66 of the candidates confirms 61 of these as…

星系天体物理 · 物理学 2021-02-24 P. Frank Winkler , Sadie C. Coffin , William P. Blair , Knox S. Long , Kip D. Kuntz

We survey four nearby irregular galaxies for radio supernova remnants (SNRs) using deep (1 sigma ~ 20 microJy), high resolution (~20 pc) VLA continuum data at 20, 6, and 3.6 cm. We identify discrete sources in these galaxies and use radio…

宇宙学与河外天体物理 · 物理学 2009-11-13 Laura Chomiuk , Eric Wilcots

We present results of a search for supernova remnants (SNRs) in archival Chandra images of M33. We have identified X-ray SNRs by comparing the list of Chandra, X-ray sources in M33 with tabulations of SNR candidates identified from (1)…

Identified radio supernova remnants (SNRs) in the Galaxy comprise an incomplete sample of the SNR population due to various selection effects. ROSAT performed the first all-sky survey with an imaging X-ray telescope, and thus provides…

We present the results of an optical search for supernova remnants (SNRs) in the nearby spiral galaxy NGC 2903. Interference filter images and spectral data were taken in March 2005 with the f/7.7 1.5 m Russian Turkish Telescope (RTT150) at…

星系天体物理 · 物理学 2009-11-13 E. Sonbas , A. Akyuz , S. Balman

We present comprehensive X-ray point source catalogs of NGC~55, NGC~2403, and NGC~4214 as part of the Chandra Local Volume Survey. The combined archival observations have effective exposure times of 56.5 ks, 190 ks, and 79 ks for NGC~55,…

Supernova remnant (SNR) candidates in the giant spiral galaxy M101 have been previously identified from ground-based H-alpha and [SII] images. We have used archival Hubble Space Telescope (HST) H-alpha and broad-band images as well as…

宇宙学与河外天体物理 · 物理学 2015-06-04 N. A. Franchetti , R. A. Gruendl , Y. -H. Chu , B. C. Dunne , T. G. Pannuti , K. D. Kuntz , C. -H. R. Chen , C. K. Grimes , T. M. Aldridge

ROSAT all-sky survey (RASS) data have provided another window to search for supernova remnants (SNRs). In reexamining this data archive, a list of unidentified extended X-ray objects have been suggested as promising SNR candidate. However,…

高能天体物理现象 · 物理学 2015-06-04 C. Y. Hui , K. A. Seo , R. H. H. Huang , L. Trepl , Y. J. Woo , T. -N. Lu , A. K. H. Kong , F. M. Walter

To date, over 220 emission nebulae in M33 have been identified as supernova remnants (SNRs) or SNR candidates, principally through [SII]:Halpha line ratios that are elevated compared to those in H II regions. In many cases, the…

星系天体物理 · 物理学 2018-04-04 Knox S. Long , William P. Blair , Dan Milisavljevic , John C. Raymond , P. Frank Winkler

In an XMM-Newton raster observation of the bright Local Group spiral galaxy M 33 we study the population of X-ray sources (X-ray binaries, supernova remnants) down to a 0.2--4.5 keV luminosity of 10^35 erg/s -- more than a factor of 10…

天体物理学 · 物理学 2009-11-10 W. Pietsch , Z. Misanovic , F. Haberl , D. Hatzidimitriou , M. Ehle , G. Trinchieri

In an analysis of XMM-Newton archival observations of the bright Local Group spiral galaxy M 31 we study the population of X-ray sources (X-ray binaries, supernova remnants) down to a 0.2-4.5 keV luminosity of 4.4E34 erg/s. EPIC hardness…

天体物理学 · 物理学 2009-11-10 W. Pietsch , M. Freyberg , F. Haberl

Narrow band images covering strong emission lines are efficient to survey supernova remnants (SNRs) in nearby galaxies. Using the narrow band images provided by the Local Group Galaxy Survey we searched for SNRs in M33. Culling the objects…

高能天体物理现象 · 物理学 2015-06-22 Jong Hwan Lee , Myung Gyoon Lee

During detailed searches for new Galactic supernova remnants (SNRs) in the Anglo Australian Observatory/United Kingdom Schmidt Telescope (AAO/UKST) HAlpha survey of the southern Galactic plane, we also uncovered, for the first time,…

星系天体物理 · 物理学 2016-12-07 M. Stupar , Q. A. Parker

A catalogue of 231 Galactic supernova remnants (SNRs) is presented, and the selection effects applicable to the identification of remnants at radio wavelengths are discussed. In addition to missing low surface brightness remnants, small…

天体物理学 · 物理学 2007-05-23 D. A. Green

We present the results of the ongoing XMM-Newton survey of M31. 17 X-ray sources detected in the survey have bright radio counterparts, and 15 X-ray sources coincide with SNR candidates from optical and radio surveys. 15 out of 17 sources…

天体物理学 · 物理学 2007-05-23 Sergey Trudolyubov , William Priedhorsky
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