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Output details

9 - Physics

University of St Andrews (joint submission with University of Edinburgh)

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Output 78 of 130 in the submission
Article title

Non-stationary dynamo and magnetospheric accretion processes of the classical T Tauri star V2129 Oph

Type
D - Journal article
Title of journal
Monthly Notices of the Royal Astronomical Society
Article number
-
Volume number
412
Issue number
4
First page of article
2454
ISSN of journal
0035-8711
Year of publication
2011
URL
-
Number of additional authors
13
Additional information

Gregory contributed throughout the paper via his theoretical interpretation of the observational data. He carried out calculations of disc truncation radii based on the new, and reanalysed archival, data; shaping the main conclusions regarding the implications for the star-disc interaction/stellar rotational evolution as the magnetic fields of young stars evolve on ~year long, and ~million-year long, timescales.

Interdisciplinary
-
Cross-referral requested
-
Research group
D - Astronomy
Citation count
27
Proposed double-weighted
No
Double-weighted statement
-
Reserve for a double-weighted output
No
Non-English
No
English abstract
-