A dataset provided by the European Space Agency

Name 090333
Title Investigating the correlation between late-time X-rays radio emission in TDEs
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0903330101

DOI https://doi.org/10.57780/esa-[xxxxxxx]
Author European Space Agency
Description The tidal disruption of a star by a black hole provides a unique opportunity to
study accretion physics. Recently, delayed radio flares have been discovered in
several TDEs, peaking years after their optical emission has faded. Various
explanations have been proposed, including off-axis jets entering our line of
sight, delayed accretion disk formation, or a state change in the accretion
flow. To elucidate the origin(s) of these flares, it has become crucial to
acquire radio and X-ray observations of these events at late-times (virgul months to
years post-discovery) to study this previously unexplored phase in the lifetime
of TDEs.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2023-04-08T01:25:45Z/2023-04-08T11:02:25Z
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 2024-05-05T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2024, Investigating The Correlation Between Late-Time X-Rays Radio Emission In Tdes, 20.10_20230417_1156, European Space Agency, https://doi.org/10.57780/esa-[xxxxxxx]