A dataset provided by the European Space Agency

Name 089220
Title The Last Gasp of the TDE Wind
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0892200101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0892200201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0892200301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0892200601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0892200701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0892200901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0892201001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0892201101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0892201201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0892201301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0892201401
...
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0892201501

DOI https://doi.org/10.57780/esa-xpksmwf
Author European Space Agency
Description When a star is tidally disrupted by a supermassive black hole, the rapid
accretion of the stellar debris may drive super-Eddington winds which. After a
period of accretion rate decay, we expect the winds to shut off, drastically
reducing the production of broad line emission and changing the evolution of the
band-specific light curve across the spectrum. Spectroscopic monitoring of new
tidal disruption events (TDEs) in the ultraviolet is the best place to observe
this transition due to the persistence of a windless disk continuum. the lack of
stellar contamination, and the wealth of high-ionization diagnostic lines that
probe the relatively small TDE accretion structure. We propose to observe 5 TDEs
over 3 epochs with monitoring UV spectroscopy and complementary X-ray and optical
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2022-08-12T21:59:14Z/2023-04-23T03:38:33Z
Version 20.10_20230417_1156
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 2024-05-09T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2024, The Last Gasp Of The Tde Wind, 20.10_20230417_1156, European Space Agency, https://doi.org/10.57780/esa-xpksmwf