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HD 15485


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2000 A UV imaging of a 6 deg diameter field around the H and Chi Persei double cluster
A stellar field centered close to the h and Chi per double cluster hasbeen observed at 2000 A by the stratospheric balloon-born telescope ofthe SCAP-2000 program. It is shown that the prevailing extinction lawproduces greater extinction at 1965 A than is predicted by the meanextinction law. The results suggest the presence of an H2 cloud in frontof h and Chi Per in the second absorbing layer and in the local arm. Agroup of hot stars centered at the same distance as the molecular cloudmay form an association of OB stars in the local arm.

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Observation and Astrometry data

Constellation:Perseus
Right ascension:02h31m34.74s
Declination:+55°17'14.8"
Apparent magnitude:8.361
Distance:242.718 parsecs
Proper motion RA:-8.2
Proper motion Dec:-7.8
B-T magnitude:8.528
V-T magnitude:8.375

Catalogs and designations:
Proper Names
HD 1989HD 15485
TYCHO-2 2000TYC 3691-1352-1
USNO-A2.0USNO-A2 1425-03547044
HIPHIP 11746

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