A dataset provided by the European Space Agency

Name 060637
Title Pulsations and long term variability of the second eclipsing HMXB in M 33
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0606370301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0606370401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0606370501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0606370601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0606370701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0606370801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0606370901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0606371001
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0606371101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0606371201
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DOI 10.5270/esa-kwnbnuq
Author Dr Wolfgang Pietsch
Description We propose 11 observations with about 3.4 day spacing of the second eclipsing high mass X-ray binary in M33. We will search for pulsations of the source down to 200ms and for an expected long term modulation of the source similar to the 35 day cycle of Her X-1. The results will allow us to decide whether the compact object in the system is a neutron star or a black hole. The Doppler delay curve of pulsations, if present, combined with the well determined orbital period could provide the mass function of the system.
Publication Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
A Deep XMM-Newton Survey of M33: Point-source Catalog, Source Detection, and Characterization of Overlapping Fields . Williams, Benjamin F., Wold, Brian, et all. . ApJS . 218-9 . 2015 . 2015ApJS..218....9W ,
Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function . Vagnetti, F., Middei, R., et all. . A&A . 593-55 . 2016 . 2016A&A...593A..55V ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Supernova remnants in M33: X-ray properties as observed by XMM-Newton . Garofali, Kristen, Williams, Benjamin F., et all. . MNRAS . 472-308 . 2017 . 2017MNRAS.472..308G ,
A New, Deep JVLA Radio Survey of M33 . White, Richard L., Long, Knox S., et all. . ApJS . 241-37 . 2019 . 2019ApJS..241...37W ,
Formation time-scales for high-mass X-ray binaries in M33 . Garofali, Kristen, Williams, Benjamin F., et all. . MNRAS . 479-3526 . 2018 . 2018MNRAS.479.3526G ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2010-01-07T13:04:04Z/2010-02-11T03:29:31Z
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 2011-03-10T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2011-03-10T00:00:00Z, 060637, 17.56_20190403_1200. https://doi.org/10.5270/esa-kwnbnuq