The SOFIA Massive (SOMA) Star Formation Survey. II. High Luminosity Protostars
Artikel i vetenskaplig tidskrift, 2019

We present multiwavelength images observed with SOFIA-FORCAST from similar to 10 to 40 mu m of seven high luminosity massive protostars, as part of the SOFIA Massive Star Formation Survey. Source morphologies at these wavelengths appear to be influenced by outflow cavities and extinction from dense gas surrounding the protostars. Using these images, we build spectral energy distributions (SEDs) of the protostars, also including archival data from Spitzer, Herschel, and other facilities. Radiative transfer (RT) models of Zhang & Tan, based on Turbulent Core Accretion theory, are then fit to the SEDs to estimate key properties of the protostars. Considering the best five models fit to each source, the protostars have masses m* similar to 12-64 M circle dot accreting at rates of m* similar to 10(-4) -10(-3) M circle dot yr(-1) inside cores of initial masses M-c similar to 100-500 M circle dot embedded in clumps with mass surface densities Sigma(cl) similar to 0.1-3 g cm(-2) and span a luminosity range of 10(4) -10(6) L circle dot. Compared with the first eight protostars in Paper I, the sources analyzed here are more luminous and, thus, likely to be more massive protostars. They are often in a clustered environment or have a companion protostar relatively nearby. From the range of parameter space of the models, we do not see any evidence that Sigma(cl) needs to be high to form these massive stars. For most sources, the RT models provide reasonable fits to the SEDs, though the cold clump material often influences the long wavelength fitting. However, for sources in very clustered environments, the model SEDs may not be such a good description of the data, indicating potential limitations of the models for these regions.

stars: formation Supporting material: data behind figures, machine-readable table

dust, extinction

infrared: stars

ISM: jets and outflows

stars: early-type

Författare

Mengyao Liu

University of Virginia

Jonathan Tan

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik, Galaktisk astrofysik

James M. De Buizer

NASA Ames Research Center

Yichen Zhang

RIKEN

Maria T. Beltran

Istituto nazionale di astrofisica (INAF)

Jan E. Staff

Univ Virgin Isl, Coll Sci & Math

Tanaka

Osaka University

National Astronomical Observatory of Japan

Barbara Whitney

University of Wisconsin Madison

Viviana Rosero

Natl Radio Astron Observ, POB O, 1003 Lopezville Rd

Astrophysical Journal

0004-637X (ISSN) 1538-4357 (eISSN)

Vol. 874 1 16

Ämneskategorier

Meteorologi och atmosfärforskning

Astronomi, astrofysik och kosmologi

Annan fysik

DOI

10.3847/1538-4357/ab07b7

Mer information

Senast uppdaterat

2019-08-20