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Last name: NEINER
First name: C.
Astronomy and Astrophysics, v. 445, p. 931-937, 2006. http://dx.doi.org/10.1051/0004-6361:20052760
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VizieR On-line Data Catalog: J/A+A, 409, p. 275 (2003)
Astron. & Astrophys., 409, pp. 275-286 (2003)
Astron. & Astrophys., 411, p. 565 (2003)
Astron. & Astrophys., 411, p. 565 (2003)
n/a, pages (2006)
n/a, pages (2006)
We analyzed the star HD 171219, one of the relatively bright Be stars observed in the seismo field of the CoRoT satellite, in order to determine its physical and pulsation characteristics. Classical Be stars are main-sequence objects of mainly B-type, whose spectra show, or have shown at some epoch, Balmer lines in emission and an infrared...
Context: Aims: In this work, we describe the pipeline for the fast supervised classification of light curves observed by the CoRoT exoplanet CCDs. We present the classification results obtained for the first four measured fields, which represent a one-year in-orbit operation. Methods: The basis of the adopted supervised classification...
Light curve parameters and classification results are presented for all the objects measured in the first four CoRoT observing runs: IRa01, SRc01, LRc01, and LRa01. The information presented here should allow scientists to make candidate lists of their objects of study and to obtain some basic light curve information. We recall that we did not...
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Communications in Asteroseismology, 156, pp. 73-87