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Direct Infall Signatures and Complex Organic Molecules toward an Isolated Embedded Protostar BHR 71

Published online by Cambridge University Press:  13 January 2020

Yao-Lun Yang
Affiliation:
Department of Astronomy, The University of Texas at Austin, USA email: yaolunyang.astro@gmail.com
Neal J. Evans II
Affiliation:
Department of Astronomy, The University of Texas at Austin, USA email: yaolunyang.astro@gmail.com Korea Astronomy and Space Science Institute, Korea Humanitas College, Kyung Hee University, Korea
Aaron Smith
Affiliation:
Department of Physics, Massachusetts Institute of Technology, USA
Joel D. Green
Affiliation:
Department of Astronomy, The University of Texas at Austin, USA email: yaolunyang.astro@gmail.com Space Telescope Science Institute, USA
Jes K. Jørgensen
Affiliation:
Centre for Star and Planet Formation, Niels Bohr Institute and Natural History Museum of Denmark, University of Copenhagen, Denmark
Jeong-Eun Lee
Affiliation:
Department of Astronomy & Space Science, Kyung Hee University, Korea
Tyler L. Bourke
Affiliation:
SKA Organization, Jodrell Bank Observatory, UK
John J. Tobin
Affiliation:
National Radio Astronomy Observatory, USA
Susan Terebey
Affiliation:
Department of Physics and Astronomy, California State University at Los Angeles, USA
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Abstract

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Our ALMA observations of HCO+ and HCN show such redshifted absorption toward an isolated core, BHR 71. Both lines show a similar redshifted absorption profile. We also found emissions of complex organic molecules (COMs) around 345 GHz from a compact region centered on the continuum source, which is barely resolved with a beam of 0″27, corresponding to ∼50 AU.

Type
Contributed Papers
Copyright
© International Astronomical Union 2020 

References

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