| Proposal ID | 030651 |
| Title | Nature of a Maser-Emitting and EGRET Source SNR: SNR-Molecular Cloud Interaction |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0306510101 |
| DOI | https://doi.org/10.5270/esa-yn0lcz1 |
| Principal Investigator, PI | Mr Hiroshi Nakajima |
| Abstract | The interaction between SNRs and molecular clouds causes immediate heating andchanges the chemical composition of the surrounding gas, emitting thermal andnon-thermal X-rays, OH maser lines, and gamma-rays. However, what causes thepartial overlap among maser-emitting SNRs, EGRET source SNRs, SNRs withparticular X-ray properties such as mixed-morphology SNRs is still unclear. CTB37A is a radio-bright Galactic SNR, and is accompanied by OH masers and EGRETsource. As the best target for the study of the SNRs in the dense conditions, wepropose the wide-band and large effective area observation of CTB 37A withXMM-Newton. |
| Publications |
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| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2006-03-01T14:22:24Z/2006-03-01T19:09:24Z |
| Version | 17.56_20190403_1200 |
| Mission Description | The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis. |
| Creator Contact | https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk |
| Date Published | 2007-05-31T00:00:00Z |
| Last Update | 2025-01-27 |
| Keywords | "chemical composition", "dense conditions", "egret source", "wide band", "oh maser lines", "maser emitting", "oh masers", "xmm newton", "partial overlap", "molecular clouds causes", "XMM-Newton", "xray properties", "supernova remnant", "nonthermal xray", "ctb 37a", "emitting thermal", "XMM", "gamma rays" |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Mr Hiroshi Nakajima, 2007, 'Nature of a Maser-Emitting and EGRET Source SNR: SNR-Molecular Cloud Interaction', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-yn0lcz1 |