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Studies in RS canum venaticorum type stars (Record no. 14492)

MARC details
000 -LEADER
fixed length control field 02314nam a2200241Ia 4500
003 - CONTROL NUMBER IDENTIFIER
control field IN-BaIIA
005 - DATE AND TIME OF LATEST TRANSACTION
control field 20211110170651.0
008 - FIXED-LENGTH DATA ELEMENTS--GENERAL INFORMATION
fixed length control field 211028s9999 xx 000 0 eng d
040 ## - CATALOGING SOURCE
Transcribing agency IIA Library
080 ## - UNIVERSAL DECIMAL CLASSIFICATION NUMBER
Universal Decimal Classification number 043:524.33
Item number MOH
100 ## - MAIN ENTRY--PERSONAL NAME
Personal name Mohin, S
9 (RLIN) 18487
Relator term Author
245 #0 - TITLE STATEMENT
Title Studies in RS canum venaticorum type stars
Remainder of title a thesis submitted for the degree of Doctor of Philosophy in the faculty of science, Punjab University, Chandigarh
Statement of responsibility, etc. S. Mohin
Medium [Ph.D Thesis]
260 ## - PUBLICATION, DISTRIBUTION, ETC.
Place of publication, distribution, etc. Bangalore
Name of publisher, distributor, etc. Indian Institute of Astrophysics
Date of publication, distribution, etc. 1992
300 ## - PHYSICAL DESCRIPTION
Extent v,165p.
500 ## - GENERAL NOTE
General note Thesis Supervisor R. K. Kochhar
502 ## - DISSERTATION NOTE
Degree type Doctor of Philosophy
Name of granting institution Indian Institute of Astrophysics, Bangalore\
Year degree granted 1992
520 ## - SUMMARY, ETC.
Summary, etc. It had been customary to divide variable stars into three classes: eruptive, pulsating, and eclipsing. It has recently been realized that there exists a fourth class of 'rotating variable stars' to which RS Canum Venaticorum systems belong. The most important characteristic of RS CVn systems in the optical region is the variable light curve arising from rotational modulation by spotted areas on the stellar photosphere. The present work was started with the aim of obtaining multiband photometric observations covering the entire phases of light curve for a few selected RS CVn stars and to use our database in conjunction with published<br/>observations to numerically model the light curves with a view to deriving physical parameters. Though RS eVn characteristics were first detected in double-lined spectroscopic binaries, later many single-lined spectroscopic binaries<br/>were found. We have selected two single-lined and two double-lined binaries for our investigation. All four are non-eclipsing close binaries: DM UMa and II Peg are single-lined, whereas V711 Tau and UX Ari are doublelined. All these objects are known to show HO:' as pure emission feature above the continuum at all times. This is a clear signature of chromospheric<br/>activity. So it was decided to supplement the photometric data with H 0'. spectroscopy. The thesis has been divided into eight chapters.
650 ## - SUBJECT ADDED ENTRY--TOPICAL TERM
Topical term or geographic name entry element Ph.D Thesis
9 (RLIN) 1344
650 ## - SUBJECT ADDED ENTRY--TOPICAL TERM
Topical term or geographic name entry element Variable Stars
9 (RLIN) 1140
700 ## - ADDED ENTRY--PERSONAL NAME
Personal name R. K. Kochhar
Relator term Supervisor
9 (RLIN) 48881
856 ## - ELECTRONIC LOCATION AND ACCESS
Uniform Resource Identifier <a href="http://prints.iiap.res.in/handle/2248/682">http://prints.iiap.res.in/handle/2248/682</a>
Link text Click Here to Access eThesis
942 ## - ADDED ENTRY ELEMENTS (KOHA)
Koha item type Thesis & Dissertations
Source of classification or shelving scheme Universal Decimal Classification
Holdings
Withdrawn status Lost status Source of classification or shelving scheme Damaged status Not for loan Home library Current library Shelving location Date acquired Full call number Barcode Date last seen Price effective from Koha item type
    Universal Decimal Classification     IIA Library-Bangalore IIA Library-Bangalore General Stacks 13/02/2002 043:524.33/ MOH 15414 05/11/2021 13/02/2002 Thesis & Dissertations

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