A dataset provided by the European Space Agency

Name 069125
Title Ring galaxies as the cradle of ULXs
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0691250101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0691250201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0691250301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0691250401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0691250501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0691250601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0691250701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0691250801

DOI https://doi.org/10.5270/esa-2th77dg
Author European Space Agency
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, Ring Galaxies As The Cradle Of Ulxs, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-2th77dg