A dataset provided by the European Space Agency

Name: DG Tau and its jet in time
Published: 2013-10-09T00:00:00Z

Proposal ID	069166
Title	DG Tau and its jet in time
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0691660401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0691660501
DOI	https://doi.org/10.5270/esa-bpnnyan
Principal Investigator, PI	Dr P. Christian Schneider
Abstract	The classical T Tauri star DG Tau drives a spectacular jet which contains plasmawith temperatures ranging from 10^4 to >10^6 K within the innermost 50 AU.Although, the luminosity of the jet related X-ray emission varies by almost afactor of two within six years, no proper-motion could be observed as for theouter emission regions of the jet. We propose to monitor the luminosityevolution with two 25 ks exposures in order to derive the timescale on whichsuch variations occur. With the large multi-wavelength campaign currentlyunderway, this represents the unique chance to relate the evolution of the softX-ray emission with other jet tracers and thus to decide whether the X-rayemission is connected to the optically observed outflow of only 10^4 K.
Publications	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 \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch, Eric W., \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F Classification of 4XMM-DR9 sources by machine learning \|Zhang, Yanxia, Zhao, Yongheng, \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions \|Pan, Zeyang, Qu, Zhijie, et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez, Antonio C., \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque, Pedro, Balaji, Shyam, \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2012-08-14T00:22:54Z/2012-09-14T21:15:20Z
Version	17.56_20190403_1200
Mission Description	The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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	2013-10-09T00:00:00Z
Keywords	"jet tracers", "dg tau", "variations occur", "outer emission region", "spectacular jet", "multi wavelength campaign", "luminosity evolution", "xray emission", "temperatures ranging", "proper motion", "soft xray emission"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr P. Christian Schneider, 2013, 'DG Tau and its jet in time', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-bpnnyan