A dataset provided by the European Space Agency

Name 060486
Title Phase-resolved X-ray study of the accreting binary T Tauri star V4046 Sgr
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604860201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604860301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0604860401

DOI 10.5270/esa-4b8pkdf
Author Dr Thierry Montmerle
Description We propose to observe the ''twin binary.. T Tauri star V4046 Sgr, to look for phase-resolved, high- resolution spectroscopic signatures of magnetic accretion. All the detectors of XMM will be used, to get access to accurate densities, temperature, and elemental abundances of the plasma in the accretion shock region, and to characterize flare emission. With the RGS, we will be able to get elemental abundances resolved down to 1-10, and density-sensitive f-i ratios down to 1-4, of the 2.4- day orbital period of the system. Taking into account the visibility gaps in the XMM orbit, *we need to observe 3 contiguous orbital periods*, giving a total exposure request of 300 ksec.
Publication The Close T Tauri Binary System V4046 Sgr: Rotationally Modulated X-Ray Emission from Accretion Shocks . Argiroffi, C., Maggio, A., et all. . ApJ . 752-100 . 2012 . 2012ApJ...752..100A ,
GSC 07396-00759 = V4046 Sgr C[D]: A Wide-separation Companion to the Close T Tauri Binary System V4046 Sgr AB . Kastner, J. H., Sacco, G. G., et all. . ApJ . 740-17 . 2011 . 2011ApJ...740L..17K ,
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 ,
Autoclassification of the Variable 3XMM Sources Using the Random Forest Machine Learning Algorithm . Farrell, Sean A., Murphy, Tara, . ApJ . 813-28 . 2015 . 2015ApJ...813...28F ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
A sensitive search for unknown spectral emission lines in the diffuse X-ray background with XMM-Newton . Gewering-Peine, A., Horns, D., . JCAP . 6-36 . 2017 . 2017JCAP...06..036G ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2009-09-15T00:57:56Z/2009-09-20T11:01:19Z
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 2010-10-13T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010-10-13T00:00:00Z, 060486, 17.56_20190403_1200. https://doi.org/10.5270/esa-4b8pkdf