Published May 20, 2016 | Version Published
Book Section - Chapter Open

Explosive Outflows from Forming Massive Stars

  • 1. ROR icon University of Colorado Boulder
  • 2. ROR icon European Southern Observatory
  • 3. ROR icon California Institute of Technology

Abstract

AO imaging of the near IR [Fe ii] and H_2 lines and ALMA CO J = 2 − 1 data confirms the explosive nature of the BN/KL outflow in Orion. N-body interactions in compact groups may be responsible for the production of powerful, explosive protostellar outflows and luminous infrared flares. The Orion event may have been triggered by a protostellar merger. First results of a search for Orion-like events in 200 nearby galaxies with the SPitzer InfraRed Intensive Transients Survey (SPIRITS) are briefly discussed.

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© 2016 EAS, EDP Sciences.

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Identifiers

Eprint ID
68907
Resolver ID
CaltechAUTHORS:20160708-080943664

Dates

Created
2016-07-09
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Updated
2021-11-11
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Series Name
EAS Publications Series
Series Volume or Issue Number
75-76