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13-colour photometry of pre-main sequence stars: preliminary report and results

Abstract

Broad (UBVRI) and intermediate (13-colour) band photometry of 160 stars selected mainly from the Herbig Rao catalogue are being carried on currently, mainly to complement the published data of these stars in the optical window (for example shortward of the Balmer and longward of the Paschen discontinuities). The 13-colour photometric system and its applications to pre-main sequences stars are briefly discussed. First results are presented.
Authors:
Chavarria-K, C; de Lara, E [1] 
  1. Universidad Nacional Autonoma de Mexico, Mexico City. Inst. de Astronomia
Publication Date:
Jan 01, 1981
Product Type:
Conference
Reference Number:
AIX-14-718575; EDB-83-037165
Resource Relation:
Journal Name: Rev. Mex. Astron. Astrofis.; (Mexico); Journal Volume: 6; Conference: 2. Latin American Regional Meeting on Astronomy, Merida (Venezuela), 19 - 23 Jan 1981
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; STARS; SPECTROPHOTOMETRY; ASTRONOMY; STAR EVOLUTION; 640102* - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources
OSTI ID:
6575183
Country of Origin:
Mexico
Language:
English
Other Identifying Numbers:
Journal ID: CODEN: RMAAD
Submitting Site:
HEDB
Size:
Pages: 159-162
Announcement Date:

Citation Formats

Chavarria-K, C, and de Lara, E. 13-colour photometry of pre-main sequence stars: preliminary report and results. Mexico: N. p., 1981. Web.
Chavarria-K, C, & de Lara, E. 13-colour photometry of pre-main sequence stars: preliminary report and results. Mexico.
Chavarria-K, C, and de Lara, E. 1981. "13-colour photometry of pre-main sequence stars: preliminary report and results." Mexico.
@misc{etde_6575183,
title = {13-colour photometry of pre-main sequence stars: preliminary report and results}
author = {Chavarria-K, C, and de Lara, E}
abstractNote = {Broad (UBVRI) and intermediate (13-colour) band photometry of 160 stars selected mainly from the Herbig Rao catalogue are being carried on currently, mainly to complement the published data of these stars in the optical window (for example shortward of the Balmer and longward of the Paschen discontinuities). The 13-colour photometric system and its applications to pre-main sequences stars are briefly discussed. First results are presented.}
journal = {Rev. Mex. Astron. Astrofis.; (Mexico)}
volume = {6}
place = {Mexico}
year = {1981}
month = {Jan}
}