A dataset provided by the European Space Agency

Proposal ID 089220
Title The Last Gasp of the TDE Wind
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DOI https://doi.org/10.57780/esa-xpksmwf
Principal Investigator, PI Dr Peter Maksym
Abstract When a star is tidally disrupted by a supermassive black hole, the rapidaccretion of the stellar debris may drive super-Eddington winds which. After aperiod of accretion rate decay, we expect the winds to shut off, drasticallyreducing the production of broad line emission and changing the evolution of theband-specific light curve across the spectrum. Spectroscopic monitoring of newtidal disruption events (TDEs) in the ultraviolet is the best place to observethis transition due to the persistence of a windless disk continuum. the lack ofstellar contamination, and the wealth of high-ionization diagnostic lines thatprobe the relatively small TDE accretion structure. We propose to observe 5 TDEsover 3 epochs with monitoring UV spectroscopy and complementary X-ray and optical
Publications
  • Discovery and follow-up of ASASSN-23bd (AT 2023clx): the lowest redshift and luminosity optically selected tidal disruption event |Hoogendam W. B. Hinkle J. T. et al. | MNRAS | 530-4501 | 2024 | 2024MNRAS.530.4501H | http://ui.adsabs.harvard.edu/#abs/2024MNRAS.530.4501H
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2022-08-12T21:59:14Z/2024-12-11T16:34:48Z
Version PPS_NOT_AVAILABLE
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 2026-01-14T00:00:00Z
Last Update 2026-07-09
Keywords XMM-Newton, OM, RGS, EPIC, X-ray, Multi-Mirror, SAS
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Peter Maksym, 2026, 'The Last Gasp of the TDE Wind', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.57780/esa-xpksmwf
Rights Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.