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A Spectroscopic Study of HL Canis Majoris
Author(s) -
Holly A. Sheets,
J. R. Thorstensen
Publication year - 2005
Publication title -
publications of the astronomical society of the pacific
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.294
H-Index - 172
eISSN - 1538-3873
pISSN - 0004-6280
DOI - 10.1086/430805
Subject(s) - astrophysics , physics , canis , astronomy , orbital period , spectroscopy , beta (programming language) , span (engineering) , stars , biology , paleontology , civil engineering , engineering , computer science , programming language
We present optical spectroscopy of the dwarf nova HL Canis Majoris over aspan of four years. The observations were made during standstill, outburst, andquiescence. We determine an orbital period of 0.2167867 +/- 0.17 days,based on radial velocities determined from H-alpha, H-beta, and He I 5876emission. We also present equivalent widths of the spectral features inoutburst and in quiescence.Comment: 4 pages, 3 postscript figures, will be published in PASP July 200

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