Reprocessing the plates of the UV bright star K1082 in the globular cluster M15 with the PDS

Details Reprocessing the plates of the UV bright star K1082 in the globular cluster M15 with the PDS Reprocessing the plates of the UV bright star K1082 in the globular cluster M15 with the PDS

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992acasn..33..383y&link_type=abstract

Acta Astronomica Sinica (ISSN 0001-5245), vol. 33, no. 4, p. 383-394.

Astronomy and Astrophysics

Astronomy

Globular Clusters, Stellar Luminosity, Stellar Magnitude, Variable Stars, Periodic Variations, Space Observations (From Earth), Ultraviolet Astronomy

Scientific paper

New variable stars in M15 were studied taking into account K1082 in CCD
frames for three nights in November 1987. Data obtained indicate with a
probability of about 90 percent that K1082 is a new variable star with
an amplitude of about 0.15 mag in 1957.

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