Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011sf2a.conf..413a&link_type=abstract
SF2A-2011: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds.: G. Alecian, K. Belkacem,
Astronomy and Astrophysics
Astrophysics
Star Formation, Pre-Main-Sequence, Intermediate-Mass Protostars, Protoplanetary Disks
Scientific paper
The study of intermediate-mass (IM) protostars is important because they provide the link between low-mass and high-mass star formation mechanisms, which are different and not well understood. To advance towards the comprehension of high-mass objects IM protostars are the next natural step. IM and high mass protostars are usually too far to be studied in detail, and their rapid evolution while they are still embedded in the parent cloud makes high-resolution radioastronomy (interferometry) a must. This work shows the most relevant results achieved by our group in the study of circumstellar disks and envelopes around IM protostars during the last few years, using IRAM instruments (30 m radiotelescope at Spain and Plateau de Bure interferometer in France) and the NRAO's Very Large Array (VLA) interferometer at USA.
Alonso-Albi Tomas
Fuente Asuncion
No associations
LandOfFree
Observational studies of intermediate-mass protostars with PdBI, 30m, and Herschel does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Observational studies of intermediate-mass protostars with PdBI, 30m, and Herschel, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observational studies of intermediate-mass protostars with PdBI, 30m, and Herschel will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1439516