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.
Accretion outbursts in massive star formation
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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.
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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.