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17 papers · 1 filter
The MUSE Data Reduction Pipeline: Status after Preliminary Acceptance Europe
Peter M. Weilbacher, Ole Streicher, Tanya Urrutia +3
MUSE, a giant integral field spectrograph, is about to become the newest facility instrument at the VLT. It will see first light in February 2014. Here, we summarize the properties…
Asymmetric features in the protoplanetary disk MWC758
M. Benisty, A. Juhasz, A. Boccaletti +25
The study of dynamical processes in protoplanetary disks is essential to understand planet formation. In this context, transition disks are prime targets because they are at an adv…
The Expanding Fireball of Nova Delphini 2013
G. H. Schaefer, T. ten Brummelaar, D. R. Gies +34
A classical nova occurs when material accreting onto the surface of a white dwarf in a close binary system ignites in a thermonuclear runaway. Complex structures observed in the ej…
Early Results from VLT-SPHERE: Long-Slit Spectroscopy of 2MASS 0122-2439B, a Young Companion Near the Deuterium Burning Limit
Sasha Hinkley, Brendan P. Bowler, Arthur Vigan +8
We present 0.95-1.80 m spectroscopy of the 12-27 companion orbiting the faint (13.6), young (120 Myr) M-dwarf 2MASS J01225093--2439505 ("2M012…
Nascent bipolar outflows associated with the first hydrostatic core candidates Barnard 1b-N and 1b-S
M. Gerin, J. Pety, A. Fuente +3
In the theory of star formation, the first hydrostatic core (FHSC) phase is a critical step in which a condensed object emerges from a prestellar core. This step lasts about one th…
The peculiar radio galaxy 4C 35.06: a case for recurrent AGN activity?
A. Shulevski, R. Morganti, P. D. Barthel +85
Using observations obtained with the LOw Fequency ARray (LOFAR), the Westerbork Synthesis Radio Telescope (WSRT) and archival Very Large Array (VLA) data, we have traced the radio…