NDLI: Quasi-Periodic Variations of Balmer Line Profiles in Spectra of the T Tau-Type Star RW Aurigae

Content Provider	Scilit
Author	Grinin, V. P. Petrov, P. P. Shakhovskaya, N. I.
Copyright Year	1983
Description	RW Aur is one of the most active T Tau-type stars with essentially variable emission line spectrum. In order to study the nature of this variability,patrol spectroscopic observations of the star were carried outfrom November 1979 to March 1982 at the 2.6-meter telescope of the Crimean Astrophysical Observatory. The spectral region λλ38OO-67OO A has been observed with a dispersion of about 40 A/mm. All nights were supplied with simultaneous spectrophotometry of the star.
Related Links	https://www.cambridge.org/core/services/aop-cambridge-core/content/view/78178AF7F0F272993E84E3B6CF30A586/S0252921100096615a.pdf/div-class-title-quasi-periodic-variations-of-balmer-line-profiles-in-spectra-of-the-t-tau-type-star-rw-aurigae-div.pdf
Ending Page	514
Page Count	2
Starting Page	513
ISSN	02529211
DOI	10.1017/s0252921100096615
Journal	International Astronomical Union Colloquium
Volume Number	71
Language	English
Publisher	Cambridge University Press (CUP)
Publisher Date	1983-01-01
Access Restriction	Open
Subject Keyword	International Astronomical Union Colloquium Astronomy and Astrophysics Spectrophotometry
Content Type	Text
Resource Type	Article

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