A dataset provided by the European Space Agency

Proposal ID 011228
Title Hot Halos and Weak Winds in Spiral Galaxies
Download Data Associated to the proposal

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112280101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112280201

DOI https://doi.org/10.5270/esa-27r3sbo
Principal Investigator, PI Dr Martin Turner
Abstract GT- Starburst galaxies are not closed systems; hot gas is seen escaping fromstarburst regions in a galactic wind. However only a few percent of galaxiesshow such high activity. What happens in typical spiral galaxies? Halos ofhot gas have been detected above the discs of normal spiral galaxies withROSAT, and there is a suggestion of weak outflows in several cases.We propose to use the EPIC spectral imagers to examine a small sample of highinclination spirals which show such plumes, in order to establish theexistence of weak galaxy winds, to measure their properties, and to map theproperties of hot galactic coronae in detail.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2002-05-27T07:15:20Z/2002-08-22T11:12:48Z
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 2003-10-04T00:00:00Z
Keywords "hot gas", "starburst galaxy", "normal spiral galaxy", "weak winds", "weak outflows", "epic spectral imagers", "typical spiral galaxy", "closed systems", "inclination spirals", "hot galactic coronae", "spiral galaxy", "starburst region", "EPIC", "weak galaxy winds", "galactic wind", "ROSAT", "hot halos"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Martin Turner, 2003, 'Hot Halos and Weak Winds in Spiral Galaxies', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-27r3sbo