A dataset provided by the European Space Agency

Name 074274
Title Search for X-ray Emission from AGB Stars in the Coronal Graveyard
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0742740101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0742740201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0742740301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0742740401

DOI https://doi.org/10.5270/esa-ctqm0ts
Author Dr Rodolfo Montez
Description Maser observations demonstrate the existence of magnetic fields in the circumstellar envelopes of AGB stars. However, thus far, only 2-3 AGB stars have exhibited evidence for coronal X-ray emission. We have demonstrated that only the sensitivity of modern X-ray telescopes can detect magnetically-induced coronal emission and have identified a sample of AGB stars which are ideal candidates to search for such emission. Specifically, we have selected a sample of AGB stars with SiO maser emission, UV emission in at least one of the GALEX bandpasses, and low mass loss rates. The four selected AGB stars provide a pilot sample that optimally probes for coronal activity beyond the giant phase and that provides valuable tests for the launching and shaping of AGB mass loss.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2014-04-16T11:32:00Z/2014-10-13T21:08:02Z
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 2015-11-03T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2015-11-03T23:00:00Z, 074274, 17.56_20190403_1200. https://doi.org/10.5270/esa-ctqm0ts