EXPORT: Near-IR observations of Vega-type and pre-main sequence stars
Eiroa, C. and Garzón, F. and Alberdi, A. and de Winter, D. and Ferlet, R. and Grady, C. A. and Cameron, A. and Davies, J. K. Joint Astronomy Center, Hilo, Hawaii, USA), and Deeg, H. J. and Harris, A. W. and Horne, K. and Merín, B. and Miranda, L. F. and Montesinos, B. and Mora, A. and Oudmaijer, R. and Palacios, J. and Penny, A. and Quirrenbach, A. and Rauer, H. and Schneider, J. and Solano, E. and Tsapras, Y. and Wesselius, P. R. (2001) EXPORT: Near-IR observations of Vega-type and pre-main sequence stars. Astronomy and Astrophysics, 365, pp. 110-114.
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We present near-IR J H K photometric data of sample of 58 main-sequence, mainly Vega-type, and pre-main sequence stars. The data were taken during four observation runs in the period May 1998 to January 1999 and form part of a coordinated effort with simultaneous optical spectroscopy and photo-polarimetry. The near-IR colors of the MS stars correspond in most cases tp photospheric colors, although noticealbe reddening is present towards a few objects, and these stars show no brightness variability within the observational errors. On the other hand, the PMS stars show near-IR excesses and variability consistent with previous data.
|Title:||EXPORT: Near-IR observations of Vega-type and pre-main sequence stars|
|Journal or Publication Title:||Astronomy and Astrophysics|
|In ISI Web of Science:||Yes|
|Page Range:||pp. 110-114|
|HGF - Research field:||Aeronautics, Space and Transport (old)|
|HGF - Program:||Space (old)|
|HGF - Program Themes:||W EW - Erforschung des Weltraums|
|DLR - Research area:||Space|
|DLR - Program:||W EW - Erforschung des Weltraums|
|DLR - Research theme (Project):||UNSPECIFIED|
|Institutes and Institutions:||Institut für Weltraumsensorik und Planetenerkundung|
|Deposited By:||elib DLR-Beauftragter|
|Deposited On:||08 Dec 2005|
|Last Modified:||14 Jan 2010 18:56|
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