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Journal article

CSI 2264: Characterizing Accretion-Burst Dominated Light Curves for Young Stars in NGC 2264

Abstract:

Based on more than four weeks of continuous high cadence photometric monitoring of several hundred members of the young cluster NGC 2264 with two space telescopes, NASA's Spitzer and the CNES CoRoT (Convection, Rotation, and planetary Transits), we provide high quality, multi-wavelength light curves for young stellar objects (YSOs) whose optical variability is dominated by short duration flux bursts, which we infer are due to enhanced mass accretion rates. These light curves show many brief -...

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Publication status:
Published

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Publisher copy:
10.1088/0004-6256/147/4/83

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Journal:
ASTRONOMICAL JOURNAL
Volume:
147
Issue:
4
Pages:
83-83
Publication date:
2014-01-26
DOI:
EISSN:
1538-3881
ISSN:
0004-6256
Source identifiers:
462741
Language:
English
Keywords:
Pubs id:
pubs:462741
UUID:
uuid:c53614f9-a0e5-47eb-973d-02b2300a841c
Local pid:
pubs:462741
Deposit date:
2014-06-17

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