REVIEW 1 cited by
Accretion outbursts in massive star formation
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
Signed reviews
read the original abstract
Using the HPC ressources of the state of Baden-W\"urttemberg, we modelled for the first time the luminous burst from a young massive star by accretion of material from its close environment. We found that the surroundings of young massive stars are shaped as a clumpy disk whose fragments provoke outbursts once they fall onto the protostar and concluded that similar strong luminous events observed in high-mass star forming regions may be a signature of the presence of such disks.
Forward citations
Cited by 1 Pith paper
-
Infrared and sub-mm observations of outbursting young stars with Herschel and Spitzer
New Herschel and Spitzer far-infrared photometry and CO spectroscopy for 12 outbursting young stars yield SEDs, CO rotational temperatures mostly near 0-100 K and 400-500 K, and evidence that HH 381 IRS is brightening.
Discussion (0). Continue with ORCID to comment.