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Detection of a Disk Surrounding the Variably Accreting Young Star HBC722

Yek, X, Dunham, MM, Arce, HG, Bourke, TL, Chen, X, Green, JD, Kospal, A and Longmore, SN (2020) Detection of a Disk Surrounding the Variably Accreting Young Star HBC722. Research Notes of the American Astronomical Association RNAAS, 4 (9). ISSN 2515-5172

Full text not available from this repository. Please see publisher or open access link below:
Open Access URL: https://doi.org/10.3847/2515-5172/abb813 (Published version)

Abstract

We present new ALMA 233 GHz continuum observations of the FU Orionis Object HBC722. With these data we detect HBC722 at millimeter wavelengths for the first time, use this detection to calculate a circumstellar disk mass of 0.024 solar masses, and discuss implications for the burst triggering mechanism.

Item Type: Article
Uncontrolled Keywords: astro-ph.GA; astro-ph.GA
Subjects: Q Science > QB Astronomy
Q Science > QC Physics
Divisions: Astrophysics Research Institute
Publisher: American Astronomical Society; IOP Publishing
Related URLs:
Date Deposited: 28 Sep 2020 11:10
Last Modified: 28 Sep 2020 11:10
DOI or Identification number: 10.3847/2515-5172/abb813
URI: https://researchonline.ljmu.ac.uk/id/eprint/13733

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