activity
20022008
most citedCoronae in the Coronet: A very deep X-ray look into a stellar nursery

59 citations · 108 across the 3 of their papers we have counts for

collaborators

9 papers

astro-ph20084 cited

Confirmation of the binary status of Cha Halpha 2 - a very young low-mass binary in Chamaeleon

T. O. B. Schmidt, R. Neuhäuser, N. Vogt +3

Neuhaeuser & Comeron (1998, 1999) presented direct imaging evidence, as well as first spectra, of several young stellar and sub-stellar M6- to M8-type objects in the Cha I dark clo…

astro-ph200759 cited

Coronae in the Coronet: A very deep X-ray look into a stellar nursery

Jan Forbrich, Thomas Preibisch

In order to study the X-ray properties of young stellar objects (YSOs), we analyze an exceptionally sensitive Chandra dataset of the Coronet cluster in the CrA star-forming region,…

astro-ph200745 cited

Simultaneous X-ray, radio, near-infrared, and optical monitoring of Young Stellar Objects in the Coronet cluster

J. Forbrich, Th. Preibisch, K. M. Menten +11

Multi-wavelength (X-ray to radio) monitoring of Young Stellar Objects (YSOs) can provide important information about physical processes at the stellar surface, in the stellar coron…

astro-ph2005

Radio and X-ray variability of Young Stellar Objects in the Coronet Cluster

Jan Forbrich, Thomas Preibisch, Karl M. Menten

The Coronet Cluster in the nearby R CrA dark cloud offers the rare opportunity to study at least four "class I" protostellar sources as well as one candidate "class 0" source, a He…

astro-ph2005

A Millimeter Continuum Survey for Massive Protoclusters in the Outer Galaxy

R. Klein, B. Posselt, K. Schreyer +2

Our search for the earliest stages of massive star formation turned up twelve massive pre-protocluster candidates plus a few protoclusters. For this search, we selected 47 FIR-brig…

astro-ph2005

Giant Planet Formation: A First Classification of Isothermal Protoplanetary Equilibria

B. Pecnik, G. Wuchterl

We present a model for the equilibrium of solid planetary cores embedded in a gaseous nebula. From this model we are able to extract an idealized roadmap of all hydrostatic states…