DOI:
10.1051/0004-6361:20000029
IAA authors:
Alberdi, A.;Deeg, H. J.;Miranda, L. F.
Authors:
Eiroa, C.;Garzón, F.;Alberdi, A.;de Winter, D.;Ferlet, R.;Grady, C. A.;Collier Cameron, A.;Davies, J. K.;Deeg, H. J.;Harris, A. W.;Horne, K.;Merín, B.;Miranda, L. F.;Montesinos, B.;Mora, A.;Oudmaijer, R.;Palacios, J.;Penny, A.;Quirrenbach, A.;Rauer, H.;Schneider, J.;Solano, E.;Tsapras, Y.;Wesselius, P. R.
Journal:
Astronomy and Astrophysics
Abstract:
We present near-IR JHK photometric data of a sample of 58 main-sequence, mainly Vega-type, and pre-main sequence stars. The data were taken during four observing 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 to photospheric colors, although noticeable 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. Tables 1 and 2 are only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strastg.fr/cgi-bin/qcat?J/A+A/365/110
URL:
https://ui.adsabs.harvard.edu/#abs/2001A&A...365..110E/abstract
Keywords:
STARS: EMISSION-LINE;BE;STARS: PRE-MAIN SEQUENCE;STARS: VARIABLE: GENERAL;INFRARED: STARS