The XMM-Newton/Chandra monitoring campaign of the Galactic center region. Description of the program and preliminary results
We present the first results of our X-ray monitoring campaign on a 1.7 square degree region centered on Sgr A* using the satellites XMM-Newton and Chandra. The purpose of this campaign is to monitor the behavior (below 10 keV) of X-ray sources (both persistent and transient) which are too faint to b...
| Main Authors: | , , , , , , , , , , , , |
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| Format: | Journal Article |
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EDP Sciences
2006
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| Online Access: | http://www.aanda.org/index.php?option=com_article&access=standard&Itemid=129&url=/articles/aa/full/2006/15/aa4129-05/aa4129-05.html http://hdl.handle.net/20.500.11937/17283 |
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| author | Wijnands, R. in't Zand, J. Rupen, M. Maccarone, T. Homan, J. Cornelisse, R. Fender, R. Grindlay, J. van der Klis, M. Kuulkers, E. Markwardt, C. Miller-Jones, James Wang, Q. |
| author_facet | Wijnands, R. in't Zand, J. Rupen, M. Maccarone, T. Homan, J. Cornelisse, R. Fender, R. Grindlay, J. van der Klis, M. Kuulkers, E. Markwardt, C. Miller-Jones, James Wang, Q. |
| author_sort | Wijnands, R. |
| building | Curtin Institutional Repository |
| collection | Online Access |
| description | We present the first results of our X-ray monitoring campaign on a 1.7 square degree region centered on Sgr A* using the satellites XMM-Newton and Chandra. The purpose of this campaign is to monitor the behavior (below 10 keV) of X-ray sources (both persistent and transient) which are too faint to be detected by monitoring instruments aboard other satellites currently in orbit (e.g., Rossi X-ray Timing Explorer; INTEGRAL). Our first monitoring observations (using the HRC-I aboard Chandra) were obtained on June 5, 2005. Most of the sources detected could be identified with foreground sources, such as X-ray active stars. In addition we detected two persistent X-ray binaries (1E 1743.1-2843; 1A 1742-294), two faint X-ray transients (GRS 1741.9-2853; XMM J174457-2850.3), as well as a possible new transient source at a luminosity of a few times 10^34 erg s-1. We report on the X-ray results on these systems and on the non-detection of the transients in follow-up radio data using the Very Large Array. We discuss how our monitoring campaign can help to improve our understanding of the different types of X-ray transients (i.e., the very faint ones). |
| first_indexed | 2025-11-14T07:20:42Z |
| format | Journal Article |
| id | curtin-20.500.11937-17283 |
| institution | Curtin University Malaysia |
| institution_category | Local University |
| last_indexed | 2025-11-14T07:20:42Z |
| publishDate | 2006 |
| publisher | EDP Sciences |
| recordtype | eprints |
| repository_type | Digital Repository |
| spelling | curtin-20.500.11937-172832017-05-30T07:59:51Z The XMM-Newton/Chandra monitoring campaign of the Galactic center region. Description of the program and preliminary results Wijnands, R. in't Zand, J. Rupen, M. Maccarone, T. Homan, J. Cornelisse, R. Fender, R. Grindlay, J. van der Klis, M. Kuulkers, E. Markwardt, C. Miller-Jones, James Wang, Q. accretion accretion disks X-rays: binaries binaries: close We present the first results of our X-ray monitoring campaign on a 1.7 square degree region centered on Sgr A* using the satellites XMM-Newton and Chandra. The purpose of this campaign is to monitor the behavior (below 10 keV) of X-ray sources (both persistent and transient) which are too faint to be detected by monitoring instruments aboard other satellites currently in orbit (e.g., Rossi X-ray Timing Explorer; INTEGRAL). Our first monitoring observations (using the HRC-I aboard Chandra) were obtained on June 5, 2005. Most of the sources detected could be identified with foreground sources, such as X-ray active stars. In addition we detected two persistent X-ray binaries (1E 1743.1-2843; 1A 1742-294), two faint X-ray transients (GRS 1741.9-2853; XMM J174457-2850.3), as well as a possible new transient source at a luminosity of a few times 10^34 erg s-1. We report on the X-ray results on these systems and on the non-detection of the transients in follow-up radio data using the Very Large Array. We discuss how our monitoring campaign can help to improve our understanding of the different types of X-ray transients (i.e., the very faint ones). 2006 Journal Article http://hdl.handle.net/20.500.11937/17283 http://www.aanda.org/index.php?option=com_article&access=standard&Itemid=129&url=/articles/aa/full/2006/15/aa4129-05/aa4129-05.html EDP Sciences restricted |
| spellingShingle | accretion accretion disks X-rays: binaries binaries: close Wijnands, R. in't Zand, J. Rupen, M. Maccarone, T. Homan, J. Cornelisse, R. Fender, R. Grindlay, J. van der Klis, M. Kuulkers, E. Markwardt, C. Miller-Jones, James Wang, Q. The XMM-Newton/Chandra monitoring campaign of the Galactic center region. Description of the program and preliminary results |
| title | The XMM-Newton/Chandra monitoring campaign of the Galactic center region. Description of the program and preliminary results |
| title_full | The XMM-Newton/Chandra monitoring campaign of the Galactic center region. Description of the program and preliminary results |
| title_fullStr | The XMM-Newton/Chandra monitoring campaign of the Galactic center region. Description of the program and preliminary results |
| title_full_unstemmed | The XMM-Newton/Chandra monitoring campaign of the Galactic center region. Description of the program and preliminary results |
| title_short | The XMM-Newton/Chandra monitoring campaign of the Galactic center region. Description of the program and preliminary results |
| title_sort | xmm-newton/chandra monitoring campaign of the galactic center region. description of the program and preliminary results |
| topic | accretion accretion disks X-rays: binaries binaries: close |
| url | http://www.aanda.org/index.php?option=com_article&access=standard&Itemid=129&url=/articles/aa/full/2006/15/aa4129-05/aa4129-05.html http://hdl.handle.net/20.500.11937/17283 |