A dataset provided by the European Space Agency

Name: Investigating Magnetic Activity in the Lowest Mass Pre-Main Sequence Stars
Published: 2016-09-16T22:00:00Z

Proposal ID	076319
Title	Investigating Magnetic Activity in the Lowest Mass Pre-Main Sequence Stars
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763190201
DOI	https://doi.org/10.5270/esa-ed50t83
Principal Investigator, PI	Dr David Principe
Abstract	The spectral type boundary that determines which very low-mass objects willeventually become M stars, vs. brown dwarfs, remains poorly constrained duringpre-main sequence evolution. High-energy observations of pre-main sequence Mstars offer a means to probe chromospheric and coronal activity due to stellarmagnetic activity, so as to help determine this boundary. However, even though amajority of stars in the solar neighborhood are of mid- to late-M type, theX-ray activity of such stars remain essentially unexplored for the important agerange 10-100 Myr. We propose to use XMM-Newton to observe 9 nearby (Dvirgul50 pc),young (age 10-100 Myr) stars of type M4-M9, to investigate the potentialdecrease in UV and X-ray luminosities for very low-mass stars at this age.
Publications	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	2015-08-29T20:39:49Z/2015-08-30T02:46:28Z
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	2016-09-16T22:00:00Z
Keywords	"xray luminosities", "myr stars", "xray activity", "XMM-Newton", "xmm newton", "investigating magnetic activity", "stellar magnetic activity", "poorly constrained", "potential decrease", "low mass stars", "age range", "XMM", "coronal activity", "low mass objects", "probe chromospheric", "spectral type boundary", "pre main sequence", "type m4 m9", "M4", "solar neighborhood", "brown dwarf"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr David Principe, 2016, 'Investigating Magnetic Activity in the Lowest Mass Pre-Main Sequence Stars', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ed50t83