A dataset provided by the European Space Agency

Name 086161
Title The Unexpected New Class of Brightest Cluster Galaxies\: Superluminous Spirals
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0861610101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0861610201

DOI https://doi.org/10.57780/esa-8hbz3on
Author Dr Akos Bogdan
Description Brightest Cluster Galaxies (BCGs) residing in the centers of galaxy clusters are
typically quenched giant ellipticals. Optical studies hinted, and our previous
XMM-Newton observations confirmed, that some superluminous disk galaxies are
BCGs. The existence of such a BCG population is at odds with our understanding
of the formation of these galaxies. Our AO-18 XMM-Newton program aimed to
confirm the presence of additional superluminous disk galaxies at the center of
galaxy clusters. However, due to soft proton flares, one of the most promising
superluminous spiral galaxy and its host cluster could not be characterized. We
request a short follow-up observation to carry out a dependable analysis of the
galaxy cluster and its superluminous spiral BCG.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2020-08-21T15:28:00Z/2021-01-17T12:42:16Z
Version 18.02_20200221_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 2022-02-04T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Akos Bogdan, 2022, 086161, 18.02_20200221_1200, European Space Agency, https://doi.org/10.57780/esa-8hbz3on