A dataset provided by the European Space Agency

Name 011300
Title XMM-RGS Spectroscopy of the Magellanic Cloud Supernova Remnant Sample.
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0113000201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0113000301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0113000401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0113000501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0113000601

DOI 10.5270/esa-7to9arn
Author Dr Albert Brinkman
Description GT- We propose to observe a sample of the supernova remnants in the Magellanic Clouds. The sample is comprised of E0102-72.3, N49, N103B, PSR0540-69.3 and 0519-69.0. These SNRs form a biased sample of the SNR population (they are drawn from the brighter and smaller ends of the distribution), but the sample spans the spectrum of origin, age and dynamical conditions: Two are type Ia, two are type II (one with a pulsar) and the other is evolved and containing a known soft gamma repeater. This set, studied using the RGS, promises unambiguous spectra and line diagnostics that provide strong clues that address the composition and physical state of the interstellar medium within the MCs, as well as that of the ejected stellar material.
Publication High-Resolution X-ray imaging and spectroscopy of N 103B . van der Heyden, K. J., Behar, E., et all. . A&A . 392-955 . 2002 . 2002A&A...392..955V ,
High mass X-ray binaries in the LMC: Dependence on the stellar population age and the ''propeller.. effect . Shtykovskiy, P., Gilfanov, M., . A&A . 431-597 . 2005 . 2005A&A...431..597S ,
Supernova Remnants in the Magellanic Clouds. IX. Multiwavelength Analysis of the Physical Structure of N49 . Bilikova, J., Williams, R. N. M., et all. . AJ . 134-2308 . 2007 . 2007AJ....134.2308B ,
Quiet but still bright: XMM-Newton observations of the soft gamma-ray repeater SGR0526-66 . Tiengo, A., Esposito, P., et all. . MNRAS . 399-74 . 2009 . 2009MNRAS.399L..74T ,
The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue . Watson, M. G., Schroder, A. C., et all. . A&A . 493-339 . 2009 . 2009A&A...493..339W ,
Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all. . A&A . 496-879 . 2009 . 2009A&A...496..879M ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
The kinematics and chemical stratification of the type Ia supernova remnant 0519-69.0. An XMM-Newton and Chandra study . Kosenko, D., Helder, E. A., ....
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-07-07T03:09:54Z/2001-09-18T01:26:07Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2003-01-04T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2003-01-04T00:00:00Z, 011300, 17.56_20190403_1200. https://doi.org/10.5270/esa-7to9arn