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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5176
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dc.contributor.authorParthasarathy, M-
dc.contributor.authorParsons, S. B-
dc.date.accessioned2010-07-13T14:05:16Z-
dc.date.available2010-07-13T14:05:16Z-
dc.date.issued1984-12-
dc.identifier.citationFuture of Ultraviolet Astronomy Based on Six Years of IUE Research, pp. 342-343en
dc.identifier.urihttp://hdl.handle.net/2248/5176-
dc.description.abstractThe Population II Cepheid pulsational variables AL Vir (P = 10.3 days) and W Vir (P = 17.3 days) were observed with IUE at two phases each. Only low-dispersion mid-UV exposures were feasible, but were sufficient to show a great range in Mg II emission behavior. The relationship to phase variation of emission in classical (Pop I) Cepheids of long period is unclear.en
dc.language.isoenen
dc.relation.urihttp://adsabs.harvard.edu/abs/1984NASCP2349..342Pen
dc.subjectCepheid variablesen
dc.subjectChemiluminescenceen
dc.subjectIUEen
dc.subjectMagnesiumen
dc.subjectPulse Time Modulationen
dc.subjectUltraviolet Spectraen
dc.subjectVariable starsen
dc.subjectCepheus constellationen
dc.subjectEmission spectraen
dc.subjectPhotosphereen
dc.subjectUltraviolet astronomyen
dc.titleMG II emission of Pop. 2 long-period Cepheidsen
dc.typeArticleen
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