activity
20022024
most citedThe XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST)

372 citations · 3k across the 72 of their papers we have counts for

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Showing 2014Show all

6 papers · 1 filter

astro-ph.SR2014★ 8 cited

A Chandra Observation of the Eclipsing Wolf-Rayet Binary CQ Cep

S. L. Skinner, S. A. Zhekov, M. Guedel +1

The short-period (1.64 d) near-contact eclipsing WN6+O9 binary system CQ Cep provides an ideal laboratory for testing the predictions of X-ray colliding wind shock theory at close…

astro-ph.SR2014★ 19 cited

X-ray emission from an FU Ori star in early outburst: HBC 722

Armin Liebhart, Manuel Guedel, Stephen Skinner +1

Aims: We conducted the first X-ray observations of the newly erupting FU Ori-type outburst in HBC 722 (V2493 Cyg) with the aim to characterize its X-ray behavior and near-stellar e…

astro-ph.SR2014

Chandra Resolves the T Tauri Binary System RW Aur

Stephen L. Skinner, Manuel Guedel

RW Aur is a multiple T Tauri system consisting of an early-K type primary (A) and a K5 companion (B) at a separation of 1.4 arcsec. RW Aur A drives a bipolar optical jet that is we…

astro-ph.HE2014★ 17 cited

A Chandra Grating Observation of the Dusty Wolf-Rayet Star WR48a

Svetozar A. Zhekov, Marc Gagne, Stephen L. Skinner

We present results of a Chandra High Energy Transmission Grating (HETG) observation of the carbon-rich Wolf-Rayet (WR) star WR48a. These are the first high-resolution spectra of th…

astro-ph.SR2014★ 1 cited

An X-ray and Infrared Survey of the Lynds 1228 Cloud Core

Stephen Skinner, Luisa Rebull, Manuel Guedel

The nearby Lynds 1228 (L1228) dark cloud at a distance of ~200 pc is known to harbor several young stars including the driving sources of the giant HH 199 and HH 200 Herbig-Haro ou…

astro-ph.SR2014★ 113 cited

Episodic Accretion in Young Stars

Marc Audard, Péter Ábrahám, Michael M. Dunham +10

In the last twenty years, the topic of episodic accretion has gained significant interest in the star formation community. It is now viewed as a common, though still poorly underst…