Star Formation in a Strongly Magnetized Cloud
Journal article, 2021

We study star formation in the Center Ridge 1 (CR1) clump in the Vela C giant molecular cloud, selected as a high column density region that shows the lowest level of dust continuum polarization-angle dispersion, likely indicating that the magnetic field is relatively strong. We observe the source with the Atacama Large Millimeter/submillimeter Array 7 m array at 1.05 and 1.3 mm wavelengths, which enable measurements of dust temperature, core mass, and astrochemical deuteration. A relatively modest number of 11 dense cores are identified via their dust continuum emission, with masses spanning from 0.17-6.7 M-circle dot. Overall CR1 has a relatively low compact dense gas fraction compared with other typical clouds with similar column densities, which may be a result of the strong magnetic field and/or the very early evolutionary stage of this region. The deuteration ratios, D-frac, of the cores, measured with N2H+(3-2) and N2D+(3-2) lines, span from 0.011-0.85, with the latter being one of the highest values yet detected. The level of deuteration appears to decrease with evolution from prestellar to protostellar phase. A linear filament, running approximately parallel with the large scale magnetic field orientation, is seen connecting the two most massive cores, each having CO bipolar outflows aligned orthogonally to the filament. The filament contains the most deuterated core, likely to be prestellar and located midway between the protostars. The observations permit measurement of the full deuteration structure of the filament along its length, which we present. We also discuss the kinematics and dynamics of this structure, as well as of the dense core population.

Author

Yu Cheng

University of Virginia

Jonathan Tan

University of Virginia

Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics

Paola Caselli

Max Planck Society

Laura Fissel

Queen's University

Hector G. Arce

Yale University

Francesco Fontani

Istituto nazionale di astrofisica (INAF)

Max Planck Institute for Extraterrestrial Physics

Matthew D. Goodson

The University of North Carolina at Chapel Hill

Mengyao Liu

University of Virginia

Nicholas Galitzk

University of California

Astrophysical Journal

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

Vol. 916 2 78

Eld ur is - den massiva stjärnbildningens utvecklingsstadier

Swedish Research Council (VR) (2017-04522), 2018-01-01 -- 2021-12-31.

Massive Star Formation through the Universe (MSTAR)

European Commission (EC) (788829), 2018-09-01 -- 2023-08-31.

Subject Categories

Meteorology and Atmospheric Sciences

Astronomy, Astrophysics and Cosmology

Atom and Molecular Physics and Optics

DOI

10.3847/1538-4357/ac043c

More information

Latest update

8/16/2021