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Characterizing the radio continuum nature of sources in the massive star-forming region W75N (B)

Rodriguez-Kamenetzky, A. (author)
Instituto de Astronomía Teórica y Experimental (IATE)
Carrasco-Gonzalez, C. (author)
Universidad Nacional Autónoma de México (UNAM),Universidad Nacional Autonoma de Mexico
Torrelles, J. M. (author)
Agencia Estatal Consejo Superior de Investigaciones Científicas,Spanish National Research Council,Institut d'Estudis Espacials de Catalunya (IEEC),Institute of Space Studies of Catalonia (IEEC)
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Vlemmings, Wouter, 1974 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Rodriguez, L. F. (author)
Universidad Nacional Autónoma de México (UNAM),Universidad Nacional Autonoma de Mexico
Surcis, G. (author)
Istituto nazionale di astrofisica (INAF)
Gomez, J. F. (author)
Agencia Estatal Consejo Superior de Investigaciones Científicas,Spanish National Research Council
Canto, J. (author)
Universidad Nacional Autónoma de México (UNAM),Universidad Nacional Autonoma de Mexico
Goddi, C. (author)
Radboud Universiteit,Radboud University,Universiteit Leiden (UL),Leiden University (UL)
Kim, J. S. (author)
Korea Astronomy and Space Science Institute
Kim, S-W (author)
Korea Astronomy and Space Science Institute
Anez-Lopez, N. (author)
Agencia Estatal Consejo Superior de Investigaciones Científicas,Spanish National Research Council,Institut d'Estudis Espacials de Catalunya (IEEC),Institute of Space Studies of Catalonia (IEEC)
Curiel, S. (author)
Universidad Nacional Autónoma de México (UNAM),Universidad Nacional Autonoma de Mexico
van Langevelde, H. J. (author)
Universiteit Leiden (UL),Leiden University (UL),Joint Institute for VLBI in Europe (JIVE)
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 (creator_code:org_t)
2020-06-20
2020
English.
In: Monthly Notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 0035-8711 .- 1365-2966. ; 496:3, s. 3128-3141
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • The massive star-forming region W75N (B) is thought to host a cluster of massive protostars (VLA 1, VLA 2, and VLA 3) undergoing different evolutionary stages. In this work, we present radio continuum data with the highest sensitivity and angular resolution obtained to date in this region, using the VLA-A and covering a wide range of frequencies (4-48 GHz), which allowed us to study the morphology and the nature of the emission of the different radio continuum sources. We also performed complementary studies with multi-epoch Very Large Array (VLA) data and Atacama Large Millimeter Array (ALMA) archive data at 1.3 mm wavelength. We find that VLA 1 is driving a thermal radio jet at scales of approximate to 0.1 arcsec (approximate to 130 au), but also shows signs of an incipient hypercompact HII region at scales of less than or similar to 1 arcsec (less than or similar to 1300 au). VLA 3 is also driving a thermal radio jet at scales of a few tenths of arcsec (few hundred of au). We conclude that this jet is shock exciting the radio continuum sources Bc and VLA 4 (obscured Herbig-Haro objects), which show proper motions moving outward from VLA 3 at velocities of approximate to 112-118 km s(-1). We have also detected three new weak radio continuum sources, two of them associated with millimetre continuum cores observed with ALMA, suggesting that these two sources are also embedded young stellar objects in this massive star-forming region.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
NATURVETENSKAP  -- Geovetenskap och miljövetenskap -- Geofysik (hsv//swe)
NATURAL SCIENCES  -- Earth and Related Environmental Sciences -- Geophysics (hsv//eng)
NATURVETENSKAP  -- Geovetenskap och miljövetenskap -- Multidisciplinär geovetenskap (hsv//swe)
NATURAL SCIENCES  -- Earth and Related Environmental Sciences -- Geosciences, Multidisciplinary (hsv//eng)

Keyword

stars: massive
HII regions
Herbig-Haro objects
radio continuum: ISM
ISM: jets and outflows
stars: protostars

Publication and Content Type

art (subject category)
ref (subject category)

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