Output details
9 - Physics
University of St Andrews (joint submission with University of Edinburgh)
Article title
Hot Gas Lines in T Tauri Stars
Type
D - Journal article
Title of journal
Astrophysical Journal Supplement Series
Article number
1
Volume number
207
Issue number
1
First page of article
-
ISSN of journal
0067-0049
Year of publication
2013
URL
-
Number of additional authors
22
Additional information
Gregory contributed to the theoretical interpretation of the morphology of a number of hot, UV, line profiles; in particular as to how certain features could form, and which line profiles were/were not consistent with the predictions of magnetospheric accretion models. He developed the arguments that multiple and/or inhomogeneous accretion columns are necessary to account for a subset of the observed line profiles. He also contributed to the comparison with literature X-ray studies of accretion onto young stars.
Interdisciplinary
-
Cross-referral requested
-
Research group
D - Astronomy
Citation count
0
Proposed double-weighted
No
Double-weighted statement
-
Reserve for a double-weighted output
No
Non-English
No
English abstract
-
