Add to ORKGThe X-ray Emission Survey of the Taurus Molecular Cloud (XEST) is an exceptionally large project to systematically investigate the high-energy properties of young stellar objects in this nearest star-forming region. It is accompanied by optical and near-infrared surveys of the same area. When XMM-Newton archival observations are added, the total X-ray exposure time is more than 200 hours shared among 25 pointings. In particular the surveyed areas, combined with two Chandra archival observations, allow us to study the X-ray emission of 19 young bona fide brown dwarfs (BDs) of the Taurus Molecular Cloud (TMC). We report here the properties of the X-ray emission of these young BDs. We detected half of this substellar sample in X-rays. Comparis...
Aims. We have analyzed optical spectra of 25 X-ray sources identified as potential new members of th...
Aims. The objective of this study is to determine the general X-ray properties of the young stars in...
We report on a 30ksec XMM-Newton observation of the central region of the Cha I star forming cloud. ...
The X-ray Emission Survey of the Taurus Molecular Cloud (XEST) is an exceptionally large project to ...
International audienceAims.We report the X-ray properties of young (~3 Myr) bona fide brown dwarfs o...
The Taurus Molecular Cloud (TMC) ranks among the nearest and best-studied low-mass star formation re...
6 pages and 4 Figures. Accepted by A&A, to appear in a special section/issue dedicated to the XMM-Ne...
We have carried out an extensive search for X-ray emission from young, very low-mass objects near an...
75 pg, 77 figs. Accepted by A&A, to appear in a special section/issue dedicated to the XMM-Newton Ex...
We have carried out an extensive search for X-ray emission from young, very low-mass objects near an...
(abridged:) The Taurus Molecular Cloud (TMC) contains numerous prototypical examples of deeply embed...
I present a summary of recent observational constraints on the accretion properties of young stars a...
International audienceAims.We aim to characterize the U-band variability of young brown dwarfs in th...
Aims. We analyze 19 bright variable X-ray sources detected in the XMM-Newton Extended Survey of the ...
We use the sensitive X-ray data from the Chandra Orion Ultradeep Project (COUP) to study the X-ray p...
Aims. We have analyzed optical spectra of 25 X-ray sources identified as potential new members of th...
Aims. The objective of this study is to determine the general X-ray properties of the young stars in...
We report on a 30ksec XMM-Newton observation of the central region of the Cha I star forming cloud. ...
The X-ray Emission Survey of the Taurus Molecular Cloud (XEST) is an exceptionally large project to ...
International audienceAims.We report the X-ray properties of young (~3 Myr) bona fide brown dwarfs o...
The Taurus Molecular Cloud (TMC) ranks among the nearest and best-studied low-mass star formation re...
6 pages and 4 Figures. Accepted by A&A, to appear in a special section/issue dedicated to the XMM-Ne...
We have carried out an extensive search for X-ray emission from young, very low-mass objects near an...
75 pg, 77 figs. Accepted by A&A, to appear in a special section/issue dedicated to the XMM-Newton Ex...
We have carried out an extensive search for X-ray emission from young, very low-mass objects near an...
(abridged:) The Taurus Molecular Cloud (TMC) contains numerous prototypical examples of deeply embed...
I present a summary of recent observational constraints on the accretion properties of young stars a...
International audienceAims.We aim to characterize the U-band variability of young brown dwarfs in th...
Aims. We analyze 19 bright variable X-ray sources detected in the XMM-Newton Extended Survey of the ...
We use the sensitive X-ray data from the Chandra Orion Ultradeep Project (COUP) to study the X-ray p...
Aims. We have analyzed optical spectra of 25 X-ray sources identified as potential new members of th...
Aims. The objective of this study is to determine the general X-ray properties of the young stars in...
We report on a 30ksec XMM-Newton observation of the central region of the Cha I star forming cloud. ...