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The Galactic Center Cloud G2—a Young Low-mass Star with a Stellar Wind

Scoville, N. and Burkert, A. (2013) The Galactic Center Cloud G2—a Young Low-mass Star with a Stellar Wind. Astrophysical Journal, 768 (2). Art. No. 108. ISSN 0004-637X. doi:10.1088/0004-637X/768/2/108. https://resolver.caltech.edu/CaltechAUTHORS:20130604-142435479

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Abstract

We explore the possibility that the G2 gas cloud falling in toward SgrA^* is the mass-loss envelope of a young T Tauri star. As the star plunges to smaller radius at 1000-6000 km s^(–1), a strong bow shock forms where the stellar wind is impacted by the hot X-ray emitting gas in the vicinity of SgrA^*. For a stellar mass-loss rate of 4 × 10^(–8) M_☉ yr^(–1) and wind velocity 100 km s^(–1), the bow shock will have an emission measure (EM = n^2 vol) at a distance ~10^(16) cm, similar to that inferred from the IR emission lines. The ionization of the dense bow shock gas is potentially provided by collisional ionization at the shock front and cooling radiation (X-ray and UV) from the post shock gas. The former would predict a constant line flux as a function of distance from SgrA^*, while the latter will have increasing emission at lesser distances. In this model, the star and its mass-loss wind should survive pericenter passage since the wind is likely launched at 0.2 AU and this is much less than the Roche radius at pericenter (~3 AU for a stellar mass of 2 M_☉). In this model, the emission cloud will probably survive pericenter passage, discriminating this scenario from others.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0004-637X/768/2/108DOIUNSPECIFIED
http://iopscience.iop.org/0004-637X/768/2/108PublisherUNSPECIFIED
ORCID:
AuthorORCID
Scoville, N.0000-0002-0438-3323
Additional Information:© 2013 American Astronomical Society. Received 2013 February 10; accepted 2013 February 25; published 2013 April 19. We would like to thank Lynne Hillenbrand for helpful discussions on the properties of TTauri stars and Andreas Eckart for suggestions. AB thanks Caltech for the hospitality of a visit which stimulated this project. We acknowledge discussions with Alessandro Ballone and Marc Schartmann who are further developing this model with detailed numerical simulation.
Subject Keywords:accretion, accretion disks; black hole physics; Galaxy: center; ISM: clouds
Issue or Number:2
DOI:10.1088/0004-637X/768/2/108
Record Number:CaltechAUTHORS:20130604-142435479
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20130604-142435479
Official Citation:The Galactic Center Cloud G2—a Young Low-mass Star with a Stellar Wind N. Scoville and A. Burkert doi:10.1088/0004-637X/768/2/108
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:38789
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:04 Jun 2013 21:36
Last Modified:09 Nov 2021 23:40

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