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  The role of interacting stellar winds feeding Sagittarius A*

Calderón, D., Cuadra, J., Schartmann, M., Burkert, A., & Russell, C. M. P. (2020). The role of interacting stellar winds feeding Sagittarius A*.

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The role of interacting stellar winds feeding Sagittarius A.pdf (Any fulltext), 795KB
 
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 Creators:
Calderón, Diego1, Author           
Cuadra, Jorge, Author
Schartmann, Marc1, Author           
Burkert, Andreas1, Author           
Russell, C. M. P., Author
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1Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society, ou_159895              

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 Abstract: The inner parsec of our Galaxy is populated by hundreds of young, massive stars. Their stellar winds fill the region with very hot (∼107 K) plasma. However, only a small fraction is accreted by the central super massive black hole, Sagittarius A*. We simulate the system of mass-losing stars feeding the black hole, finding that material can accumulate around it as a disk-like structure, provided it is modelled for long enough timescales (t > 3000 yr).

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Language(s): eng - English
 Dates: 2020
 Publication Status: Issued
 Pages: -
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 Table of Contents: -
 Rev. Type: Peer
 Identifiers: Other: LOCALID: Reihe: Astron..528, p.221-222
URI: http://www.aspbooks.org/a/volumes/article_details/?paper_id=40082
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Title: New Horizons in Galactic Center Astronomy and Beyond
Place of Event: Keio University, Yokohama, Japan
Start-/End Date: 2019-10-21 - 2019-10-24

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Title: Galactic center workshop 2019: New Horizons in Galactic Center Astronomy and Beyond
Source Genre: Multi-Volume
 Creator(s):
Masato , Tsuboi, Author
Tomoharu , Oka, Author
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-
Publ. Info: -
Pages: - Volume / Issue: - Sequence Number: - Start / End Page: - Identifier: ISBN: 978-1-58381-943-2
ISBN: 978-1-58381-944-9

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Title: Astronomical Society of the Pacific Conference Series
  Other : ASP Conference Series
Source Genre: Series
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Publ. Info: San Francisco, CA, USA : Astronomical Society of the Pacific
Pages: - Volume / Issue: 528 Sequence Number: - Start / End Page: 221 - 222 Identifier: ISSN: 1050-3390