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Accretion dynamics and disk evolution in NGC 2264: a study based on the Corot photometric observations

Abstract:

The young cluster NGC 2264 was observed with the Corot satellite for 23 days uninterruptedly in March 2008 with unprecedent photometric accuracy. We present here the first results of the analysis of the accreting population. We intended to look for possible light curve variability of the same nature as that observed in the classical T Tauri star AA Tau, which was attributed to a magnetically controlled inner disk warp, which is directly associated with the interaction between the stellar magn...

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Publication status:
Published

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Publisher copy:
10.1051/0004-6361/201014184

Authors


Alencar, SHP More by this author
Teixeira, PS More by this author
Guimaraes, MM More by this author
McGinnis, PT More by this author
Gameiro, JF More by this author
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Journal:
ASTRONOMY and ASTROPHYSICS
Volume:
519
Issue:
9
Pages:
A88-A88
Publication date:
2010-05-24
DOI:
EISSN:
1432-0746
ISSN:
0004-6361
URN:
uuid:476f5216-8e13-404f-86a5-20baf0878fe2
Source identifiers:
159054
Local pid:
pubs:159054
Language:
English
Keywords:

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