Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4411
Title: Orbit of the spectroscopic binary B Persei
Authors: Rajamohan, R
Parthasarathy, M
Keywords: Binary Stars;Orbital Elements;Stellar Motions;Stellar Spectrophotometry;Apsides;Emission Spectra;Mass Transfer;Radial Velocity;Radio Sources (Astronomy)
Issue Date: Apr-1975
Publisher: Indian Academy of Sciences
Citation: Pramana - Journal of Physics, Vol. 4, No. 4, pp. 153 - 159
Abstract: Spectroscopic orbital elements are derived for the close binary system b Persei on the basis of forty spectrograms. The period is redetermined as 1.527360 days, and variations in the orbital elements are confirmed by reanalyzing previous observations. It is shown that variations in some of these elements may result from distortion of the radial-velocity curve by gas streams in the system. It is suggested that b Persei is in an active mass-transfer stage.
URI: http://hdl.handle.net/2248/4411
ISSN: 0304-4289
???metadata.dc.relation.uri???: http://adsabs.harvard.edu/abs/1975Prama...4..153R
http://www.ias.ac.in/j_archive/pramana/4/vol4contents.html
Appears in Collections:IIAP Publications

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