Name | 069125 |
Title | Ring galaxies as the cradle of ULXs |
URL | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0691250101 |
DOI | https://doi.org/10.5270/esa-2th77dg |
Author | Dr Anna Wolter |
Description | Ring galaxies are unique laboratories to study the effects of galaxy interactions: they are characterized by high SFR,enhanced X-ray emission, and large number of ULXs. However only 4 source are published. We selected all collisional rings at z<0.02 from the Arp&Madore sample of southern ring galaxies for a statistical sample of 12. As a first step we ask for XMM-Newton snapshots of 8 galaxies that suit the XMM-Newton characteristics. We expect to detect the ring as a bright X-ray source, to which both gas and point sources (mostly ULXs) contribute. The non-detection of X-ray sources would represent an unexpected and important discovery, indicating that known the sources are quite different from the rest of the population. |
Publication | No observations found associated with the current proposal |
Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2012-05-04T09:50:56Z/2013-04-02T20:55:49Z |
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 | 2014-04-16T00:00:00Z |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, 2014-04-16T00:00:00Z, 069125, 17.56_20190403_1200. https://doi.org/10.5270/esa-2th77dg |