activity
19982009
most citedThe XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST)

372 citations · 1.7k across the 27 of their papers we have counts for

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Showing 2003Show all

6 papers · 1 filter

astro-ph2003

Population and dynamical state of the eta Chamaeleontis sparse young open cluster

A-Ran Lyo, Warrick A. Lawson, Eric D. Feigelson +1

We report new results in our continuing study of the unique compact (1 pc extent), nearby (d = 97 pc), young (t = 9 Myr) stellar cluster dominated by the B9 star eta Chamaeleontis.…

astro-ph2003

The epsilon Chamaeleontis young stellar group and the characterization of sparse stellar clusters

Eric D. Feigelson, Warrick A. Lawson, Gordon P. Garmire

We present the outcomes of a Chandra X-ray Observatory snapshot study of five nearby Herbig Ae/Be (HAeBe) stars which are kinematically linked with the Oph-Sco-Cen Association (OSC…

astro-ph2003

Determination of the gas-to-dust ratio in nearby dense clouds using X-ray absorption measurements

MyHa Vuong, Thierry Montmerle, Nicolas Grosso +3

We present a comparison of the gas and dust properties of the dense interstellar matter in six nearby star-forming regions (d<500 pc): rho Oph, Cha I, R CrA, IC 348, NGC 1333, and…

astro-ph2003

Ten Million Degree Gas in M 17 and the Rosette Nebula: X-ray Flows in Galactic H II Regions

L. K. Townsley, E. D. Feigelson, T. Montmerle +3

We present the first high-spatial-resolution X-ray images of two high-mass star forming regions, the Omega Nebula (M 17) and the Rosette Nebula (NGC 2237--2246), obtained with the…

astro-ph2003

Coronal X-ray emission from an intermediate-age brown dwarf

Yohko Tsuboi, Yoshitomo Maeda, Eric D. Feigelson +4

We report the X-ray detection of the brown dwarf (BD) companion TWA 5B in a Myr old pre-main sequence binary system. We clearly resolve the faint companion (35 photons)…

astro-ph2003

A Deep Chandra Catalog of X-ray Point Sources toward the Galactic Center

M. P. Muno, F. K. Baganoff, M. W. Bautz +7

(abridged) We present a catalog of 2357 point sources detected during 590 ks of Chandra observations of the 17-by-17 arcminute field around Sgr A*. This field encompasses a physica…