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IS HR 1469 = NSV 1671 A Constant Star?


Arthur J. Bradley

Hubble Space Telescope Operations, NASA Goddard Space Flight Center, Greenbelt, MD 20771


Dorrit Hoffleit

Imants Platais

Department of Astronomy, Yale University, New Haven, CT 06520-8101


Presented at the October 1993 Meeting




A revised interpretation of the possible fade in brightness of star HR 1469 observed by the Hubble Space Telescope Fixed Head Star Trackers is given. Most likely HR 1469 was at a normal brightness on the reported epoch of observation.


Link to ADS abstract, article and citation information

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