activity
19992022
most citedThe Hot and Energetic Universe: A White Paper presenting the science theme motivating the Athena+ mission

395 citations · 5.2k across the 79 of their papers we have counts for

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astro-ph2008★ 134 cited

X-ray hiccups from SgrA* observed by XMM-Newton. The second brightest flare and three moderate flares caught in half a day

D. Porquet, N. Grosso, P. Predehl +14

[truncated] In Spring 2007, we observed SgrA* with XMM with a total exposure of ~230ks. We have performed timing and spectral analysis of the new X-ray flares detected during this…

astro-ph2007★ 85 cited

X-ray properties of protostars in the Orion Nebula

L. Prisinzano, G. Micela, E. Flaccomio +8

The origin and evolution of the X-rays in very young stellar objects (YSOs) are not yet well understood since it is very hard to observe YSOs in the protostellar phase. We study th…

astro-ph2007★ 1 cited

Accretion and Outflow-Related X-Rays in T Tauri Stars

M. Guedel, K. Briggs, K. Arzner +22

We report on accretion- and outflow-related X-rays from T Tauri stars, based on results from the "XMM-Newton Extended Survey of the Taurus Molecular Cloud." X-rays potentially form…

astro-ph2007★ 10 cited

X-rays from young stars - a summary of highlights from the XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST)

M. Guedel

The XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST) is a survey of the nearest large star-forming region, the Taurus Molecular Cloud (TMC), making use of all instru…

astro-ph2007★ 30 cited

Observation of enhanced X-ray emission from the CTTS AA Tau during a transit of an accretion funnel

Nicolas Grosso, Jérôme Bouvier, Thierry Montmerle +3

AA Tau was observed for about 5h per XMM orbit (2 days) over 8 successive orbits, which covers two optical eclipse periods (8.2 days). The XMM optical/UV monitor simultaneously pro…

astro-ph2007★ 13 cited

A 100ks XMM-Newton view of the Seyfert 1.8 ESO113-G010. I. Discovery of large X-ray variability and study of the FeKalpha line complex

Delphine Porquet, Phil Uttley, James N. Reeves +6

(Abridged) We present here a long (100ks) XMM-Newton follow-up of the Seyfert 1.8 galaxy ESO113-G010 performed in November 2005, in order to study over a longer time-scale its main…

astro-ph2007★ 28 cited

The X-ray activity-rotation relation of T Tauri stars in Taurus-Auriga

K. R. Briggs, M. Guedel, A. Telleschi +9

The Taurus-Auriga star-forming complex hosts the only population of T Tauri stars in which an anticorrelation of X-ray activity and rotation period has been observed. We have used…

astro-ph2006

X-ray emission and the incidence of magnetic fields in the massive stars of the Orion Nebula Cluster

V. Petit, G. A. Wade, T. Montmerle +3

Magnetic fields have been frequently invoked as a likely source of variability and confinement of the winds of massive stars. To date, the only magnetic field detected in O-type st…

astro-ph2006★ 31 cited

The XMM-Newton Optical Monitor Survey of the Taurus Molecular Cloud

Marc Audard, Kevin Briggs, Nicolas Grosso +4

The Optical Monitor (OM) on-board XMM-Newton obtained optical/ultraviolet data for the XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST), simultaneously with the X-ra…

astro-ph2006★ 372 cited

The XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST)

M. Guedel, K. R. Briggs, K. Arzner +18

(abridged:) The XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST) surveys the most populated ~5 square degrees of the Taurus star formation region, using the XMM-Newt…

astro-ph2006★ 11 cited

A U-band survey of brown dwarfs in the Taurus Molecular Cloud with the XMM-Newton Optical/UV Monitor

Nicolas Grosso, Marc Audard, Jérôme Bouvier +4

We aim to characterize the U-band variability of young brown dwarfs in the Taurus Molecular Cloud and discuss its origin. We used the XMM-Newton Extended Survey of the Taurus Molec…

astro-ph2006★ 44 cited

X-ray emission from the young brown dwarfs of the Taurus Molecular Cloud

N. Grosso, K. R. Briggs, M. Guedel +9

The XMM-Newton Extended Survey of the TMC (XEST) is a large program designed to systematically investigate the X-ray properties of young stellar/substellar objects in the TMC. In p…

astro-ph2006

X-rays from HH210 in the Orion nebula

Nicolas Grosso, Eric D. Feigelson, Konstantin V. Getman +3

We report the detection during the Chandra Orion Ultradeep Project (COUP) of two soft, constant, and faint X-ray sources associated with the Herbig-Haro object HH210. HH210 is loca…

astro-ph2005★ 29 cited

Discovery of X-ray eclipses from the transient source CXOGC J174540.0-290031 with XMM-Newton

D. Porquet, N. Grosso, G. Belanger +4

We present the XMM-Newton observations obtained during four revolutions in Spring and Summer 2004 of CXOGC J174540.0-290031, a moderately bright transient X-ray source, located at…

astro-ph2005★ 58 cited

X-ray Emission from Orion Nebula Cluster Stars with Circumstellar Disks and Jets

Joel H. Kastner, Geoffrey Franz, Nicolas Grosso +5

We investigate the X-ray and near-infrared emission properties of a sample of pre-main sequence (PMS) stellar systems in the Orion Nebula Cluster (ONC) that display evidence for ci…

astro-ph2005★ 229 cited

Global X-ray properties of the Orion Nebula region

Eric D. Feigelson, Konstantin Getman, Leisa Townsley +6

Based on the Chandra Orion Ultradeep Project (COUP) observation, we establish the global X-ray properties of the stellar population associated with the Orion Nebula. Three componen…

astro-ph2005★ 67 cited

X-ray emission from young brown dwarfs in the Orion Nebula Cluster

Thomas Preibisch, Mark J. McCaughrean, Nicolas Grosso +8

We use the sensitive X-ray data from the Chandra Orion Ultradeep Project (COUP) to study the X-ray properties of 34 spectroscopically-identified brown dwarfs with near-infrared spe…

astro-ph2005

COUP census of X-ray stars in BN-KL and OMC-1S

N. Grosso, E. D. Feigelson, K. V. Getman +11

We present a study of the X-ray sources detected in the vicinity of two density peaks in the Orion Molecular Cloud 1 (OMC-1) behind the Orion Nebula Cluster (ONC), as seen in the e…

astro-ph2005★ 28 cited

Enhanced X-ray variability from V1647 Ori, the young star in outburst illuminating McNeil's Nebula

N. Grosso, J. H. Kastner, H. Ozawa +5

We report a ~38 ks X-ray observation of McNeil's Nebula obtained with XMM on 2004 April 4. V1647 Ori, the young star in outburst illuminating McNeil's Nebula, is detected with XMM…

astro-ph2004★ 87 cited

Iron Fluorescent Line Emission from Young Stellar Objects in the Orion Nebula

M. Tsujimoto, E. D. Feigelson, N. Grosso +5

We present the result of a systematic search for the iron Kalpha fluorescent line at 6.4 keV among 1616 X-ray sources detected by ultra-deep Chandra observations of the Orion Nebul…

astro-ph2004★ 391 cited

Chandra Orion Ultradeep Project: Observations and Source Lists

K. V. Getman, E. Flaccomio, P. S. Broos +21

We present a description of the data reduction methods and the derived catalog of more than 1600 X-ray point sources from the exceptionally deep January 2003 Chandra X-ray Observat…

astro-ph2004★ 77 cited

An X-ray Outburst from the Rapidly Accreting Young Star That Illuminates McNeil's Nebula

J. H. Kastner, M. Richmond, N. Grosso +6

Young, low-mass stars are luminous X-ray sources whose powerful X-ray flares may exert a profound influence over the process of planet formation. The origin of such emission is unc…

astro-ph2004★ 52 cited

The X-ray emission from Young Stellar Objects in the rho Ophiuchi cloud core as seen by XMM-Newton

H. Ozawa, N. Grosso, T. Montmerle

We observed the main core F of the rho Ophiuchi cloud, an active star-forming region located at ~140 pc, using XMM-Newton with an exposure of 33 ks. We detect 87 X-ray sources with…

astro-ph2004★ 34 cited

Chandra observation of an unusually long and intense X-ray flare from a young solar-like star in M78

N. Grosso, T. Montmerle, E. D. Feigelson +1

LkHA312 has been observed serendipitously with the ACIS-I detector on board Chandra with 26h continuous exposure. This H_alpha emission line star belongs to the star-forming region…