The SOFIA Massive (SOMA) Radio Survey. II. Radio Emission from High-luminosity Protostars
Artikel i vetenskaplig tidskrift, 2026
We present centimeter continuum observations of seven high-luminosity massive protostars and their surrounding sources in regions with multiple targets, as part of the SOFIA Massive (SOMA) Star Formation Survey. With data from the Very Large Array and the Australia Telescope Compact Array, we analyze the spectral index, morphology, and multiplicity of the detected radio sources. The high-sensitivity, high-resolution observations allow us to resolve many sources; 65% of the reported sources are resolved at least within the synthesized beam. We report 15 new detections, 13 of which are entirely new, and 2 have counterparts at other wavelengths but are detected here for the first time at radio frequencies. We use the observations to build radio spectral energy distributions to calculate spectral indices. With radio morphologies and the spectral indices, we give assessments on the nature of the sources, highlighting six sources that display a radio jetlike morphology and a spectral index consistent with ionized jets. Combining with the SOMA Radio I sample, we present the radio–bolometric luminosity relation, especially probing the regime from L bol ∼ 104 to 106 L ⊙. Here, we find a steep rise in radio luminosity, which is expected by models that transition from shock ionization to photoionization.
Författare
Francisco Sequeira-Murillo
University of Wisconsin Madison
Viviana Rosero
National Radio Astronomy Observatory
Space Science Institute
California Institute of Technology (Caltech)
J. Marvil
National Radio Astronomy Observatory
Jonathan Tan
Chalmers, Fysik, Subatomär, högenergi- och plasmafysik
University of Virginia
Rubén Fedriani
Consejo Superior de Investigaciones Científicas (CSIC)
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Yichen Zhang
Shanghai Jiao Tong University
University of Virginia
Azia Robinson
Agnes Scott College
Prasanta Gorai
Universitetet i Oslo
Kei E.I. Tanaka
Institute of Science Tokyo
James M. De Buizer
SETI Institute
M. T. Beltrán
Osservatorio Astrofisico di Arcetri
Ryan D. Boyden
University of Virginia
Astrophysical Journal
0004-637X (ISSN) 1538-4357 (eISSN)
Vol. 996 2 119Massive Star Formation through the Universe (MSTAR)
Europeiska kommissionen (EU) (EC/H2020/788829), 2018-09-01 -- 2023-08-31.
Ämneskategorier (SSIF 2025)
Astronomi, astrofysik och kosmologi
DOI
10.3847/1538-4357/ae10bb