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Title: Coordinated optical and ultraviolet observations of DH Leo

Abstract

Results are reported from contemporaneous KPNO optical spectroscopy, IUE UV spectroscopy, and KPNO R photometry of the DH Leo triple system in spring 1987. The data are presented in tables, graphs, and spectral phase images and discussed in detail. The H-alpha, H-beta, H-gamma, H-delta, and Ca II H and IRT lines are found to have excess emission, and the phase modulation in H-alpha, H-beta, and Ca II is well correlated with the photometric modulation. This result is attributed to the combination of (1) a small amount of global chromospheric emission and (2) emission from plagelike regions associated with cool starspots. The (H-alpha)/(H-beta) ratio is found to be significantly lower than that in longer-period RS CVn systems. 22 refs.

Authors:
; ; ; ;  [1]
  1. Pennsylvania State Univ., University Park (USA) Kitt Peak National Observatory, Tucson, AZ (USA)
Publication Date:
OSTI Identifier:
6439910
Resource Type:
Journal Article
Journal Name:
Astronomical Journal; (USA)
Additional Journal Information:
Journal Volume: 100; Journal ID: ISSN 0004-6256
Country of Publication:
United States
Language:
English
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; BINARY STARS; ULTRAVIOLET SPECTRA; VISIBLE SPECTRA; BALMER LINES; EMISSION SPECTRA; GRAPHS; IMAGES; MORPHOLOGY; PHOTOMETRY; SPECTROSCOPY; STARSPOTS; TABLES; SPECTRA; STARS; STELLAR ACTIVITY; 640102* - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources

Citation Formats

Newmark, J S, Buzasi, D L, Huenemoerder, D P, Ramsey, L W, and Barden, S C. Coordinated optical and ultraviolet observations of DH Leo. United States: N. p., 1990. Web. doi:10.1086/115539.
Newmark, J S, Buzasi, D L, Huenemoerder, D P, Ramsey, L W, & Barden, S C. Coordinated optical and ultraviolet observations of DH Leo. United States. https://doi.org/10.1086/115539
Newmark, J S, Buzasi, D L, Huenemoerder, D P, Ramsey, L W, and Barden, S C. 1990. "Coordinated optical and ultraviolet observations of DH Leo". United States. https://doi.org/10.1086/115539.
@article{osti_6439910,
title = {Coordinated optical and ultraviolet observations of DH Leo},
author = {Newmark, J S and Buzasi, D L and Huenemoerder, D P and Ramsey, L W and Barden, S C},
abstractNote = {Results are reported from contemporaneous KPNO optical spectroscopy, IUE UV spectroscopy, and KPNO R photometry of the DH Leo triple system in spring 1987. The data are presented in tables, graphs, and spectral phase images and discussed in detail. The H-alpha, H-beta, H-gamma, H-delta, and Ca II H and IRT lines are found to have excess emission, and the phase modulation in H-alpha, H-beta, and Ca II is well correlated with the photometric modulation. This result is attributed to the combination of (1) a small amount of global chromospheric emission and (2) emission from plagelike regions associated with cool starspots. The (H-alpha)/(H-beta) ratio is found to be significantly lower than that in longer-period RS CVn systems. 22 refs.},
doi = {10.1086/115539},
url = {https://www.osti.gov/biblio/6439910}, journal = {Astronomical Journal; (USA)},
issn = {0004-6256},
number = ,
volume = 100,
place = {United States},
year = {Wed Aug 01 00:00:00 EDT 1990},
month = {Wed Aug 01 00:00:00 EDT 1990}
}