Models of Planets and Brown Dwarfs in Mira Winds
Author(s) -
Curtis Struck,
Babak E. Cohanim,
L. A. Willson
Publication year - 2002
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/341485
Subject(s) - planet , physics , brown dwarf , maser , astrophysics , astronomy , atmosphere (unit) , accretion (finance) , observable , meteorology , quantum mechanics
We present numerical hydrodynamical models of the effects of planets or browndwarfs orbiting within the extended atmosphere and wind formation zone of Miravariables. We find time-dependent wake dynamics and episodic accretionphenomena which may give rise to observable optical events and affect SiO maseremission.Comment: 4 pages, 3 figures, follow-up to JAAVSO pape
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