A dataset provided by the European Space Agency

Name 011254
Title GT Observations of Hot Stars: Tau Sco
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112540101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112540201

DOI 10.5270/esa-0urww68
Author Dr Albert Brinkman
Description GT-Tau Sco is an OB star which shows OVI superionization caused by X-ray ionization and the Auger Ionization effect. It has a large Lx-Lbol ratio (of about 10E-6) and an unusually hard X-ray spectrum. It has been suggested that clumps form in the stellar wind, stagnate and fall inward. Because of the high shock velocity that this model predicts, the temperatures in the wind can be unusually hard: high enough that the XMM spectra should show lines of ionization stages that can place strong constraints on the structure of the X-ray forming regions of the star.
Publication High-resolution X-ray spectroscopy of tau Scorpii (B0.2V) with XMM-Newton . Mewe, R., Raassen, A. J. J., et all. . A&A . 398-203 . 2003 . 2003A&A...398..203M ,
The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue . Watson, M. G., Schroder, A. C., et all. . A&A . 493-339 . 2009 . 2009A&A...493..339W ,
Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all. . A&A . 496-879 . 2009 . 2009A&A...496..879M ,
High-resolution XMM-Newton X-ray spectra of tau SCORPII . Mewe, R., Raassen, A. J. J., et all. . AdSpR . 32-1167 . 2003 . 2003AdSpR..32.1167M ,
General X-ray properties of hot, massive stars . Naze, Yael, . BSRSL . 80-109 . 2011 . 2011BSRSL..80..109N ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
Hot stars observed by XMM-Newton. I. The catalog and the properties of OB stars . Naze, Y., . A&A . 506-1055 . 2009 . 2009A&A...506.1055N ,
A report on the X-ray properties of the tau Sco-like stars . Ignace, R., Oskinova, L. M., . MNRAS . 429-516 . 2013 . 2013MNRAS.429..516I ,
X-Ray Emission from Magnetic Massive Stars . Naze, Yael, Petit, Veronique, et all. . ApJS . 215-10 . 2014 . ...,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Analysis of the X-ray emission of OB stars II: B stars . Ryspaeva, Elizaveta, Kholtygin, Alexander, . RAA . 19-120 . 2019 . 2019RAA....19..120R ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2001-08-20T00:10:11Z/2001-08-20T09:39:05Z
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 2002-09-22T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2002-09-22T00:00:00Z, 011254, 17.56_20190403_1200. https://doi.org/10.5270/esa-0urww68