A dataset provided by the European Space Agency

Name: Can brown dwarfs form in isolationquestionMark The neighborhood of FU Tau
Published: 2013-03-03T00:00:00Z

Proposal ID	067084
Title	Can brown dwarfs form in isolation? The neighborhood of FU Tau
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670840101
DOI	https://doi.org/10.5270/esa-q3g8t9f
Principal Investigator, PI	Dr Sonali Shukla
Abstract	Some theories for the formation of brown dwarfs require dynamical interactionswith young stars in order to create brown dwarfs. The recent discovery of FUTau, a brown dwarf binary seemingly born in isolation, suggests that suchdynamical interactions may not be essential for the birth of brown dwarfs. Wepropose to verify whether this system formed alone by using XMM-Newton to searchfor previously undiscovered young stars in the vicinity of FU Tau.
Publications	The enigmatic young brown dwarf binary FUTau: accretion and activity \|Stelzer, B., Scholz, A., et al. \| MNRAS \| 408-1095 \| 2010 \| 2010MNRAS.408.1095S \| http://ui.adsabs.harvard.edu/#abs/2010MNRAS.408.1095S 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	2012-02-18T14:34:31Z/2012-02-19T01:17:54Z
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	2013-03-03T00:00:00Z
Keywords	"system formed", "XMM", "xmm newton", "dynamical interactions", "brown dwarf", "XMM-Newton", "fu tau", "create brown dwarf", "brown dwarf form"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Sonali Shukla, 2013, 'Can brown dwarfs form in isolationquestionMark The neighborhood of FU Tau', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-q3g8t9f