A dataset provided by the European Space Agency

Proposal ID 015226
Title A Highly Unusual Nonthermal Shell -- X-ray Binary System in IC 10
Download Data Associated to the proposal

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0152260101

DOI https://doi.org/10.5270/esa-0wq4nsl
Principal Investigator, PI Dr Rosa Williams
Abstract We propose to examine the nearest starburst galaxy, IC 10, with particular emphasis on a large, distinct shell of nonthermal radio emission. XMM-Newton observations will be used to distinguish between three possible scenarios for the formation of this shell: outflow from a luminous X-ray binary; enhancement of superbubble emission by a recent event; or a one-time input from a massive explosion. The results are expected to add to our knowledge of the distribution of heavy elements and hot gas from massive-stars and supernovae within a galaxy; and possibly provide clues to other energetic features such as HI shells and gamma-ray bursts.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2003-07-03T17:59:40Z/2003-07-04T06:38:19Z
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 2004-08-02T00:00:00Z
Keywords "hot gas", "starburst galaxy", "time input", "massive explosion", "XMM", "luminous xray binary", "gamma ray bursts", "massive stars", "superbubble emission", "XMM-Newton", "hi shells", "nonthermal radio emission", "distinct shell", "heavy elements", "xmm newton"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Rosa Williams, 2004, 'A Highly Unusual Nonthermal Shell -- X-ray Binary System in IC 10', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-0wq4nsl