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NSV 01450: a New Bright Classical Cepheid in the Milky Way Field

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Abstract

Photometric data extracted from more than 5000 CCD observations of theMilky Way field star NSV 01450, with galactic co-ordinates l =145°.9and b=4° .9, show that this object is a bright classical Cepheid witha period of 12.639 ± 0.020 days and an average 〈 V 〉magnitude of 11.045± 0.016. The computed colour excess is E(B-V)= 0.553± 0.056, yielding a distance modulus m V -MV of 15.537 ± 0.212.In addition, it was found that the star GSC 3730_0797 in the field ofNSV 01450 is also variable.

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  1. Esteve Duran Observatory Foundation, c/ Montseny 46, 08553, Seva, Barcelona, Spain

    Enrique García-Melendo

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  1. Enrique García-Melendo
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García-Melendo, E. NSV 01450: a New Bright Classical Cepheid in the Milky Way Field. Astrophysics and Space Science 275, 479–484 (2001). https://doi.org/10.1023/A:1002819530411

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  • DOI: https://doi.org/10.1023/A:1002819530411

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