Radiative-transfer modelling of funnel flows
2007 ◽
Vol 3
(S243)
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pp. 83-94
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Made In
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AbstractEmission line profiles from pre-main-sequence objects accreting via magnetically-controlled funnel flows encode information on the geometry and kinematics of the material on stellar radius scales. In order to extract this information it is necessary to perform radiative-transfer modelling of the gas to produce synthetic line profiles. In this review I discuss the physics that needs to be included in such models, and the numerical methods and assumptions that are used to render the problem tractable. I review the progress made in the field over the last decade, and summarize the main successes and failures of the modelling work.
2003 ◽
Vol 210
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pp. 93-105
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1998 ◽
Vol 167
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pp. 209-212
1994 ◽
Vol 144
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pp. 421-426
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1994 ◽
Vol 222
(1-2)
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pp. 91-106
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1984 ◽
Vol 80
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pp. 145-151
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2017 ◽
Vol 34
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Keyword(s):
2013 ◽
Vol 9
(S304)
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pp. 407-408
2009 ◽
Vol 5
(S266)
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pp. 29-34
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