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HD 32660


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Photometry of the Eclipsing Binary FK Orionis
Not Available

Far-ultraviolet stellar photometry: A field in Orion
Far-ultraviolet photometry for 625 objects in Orion is presented. Thesedata were extracted from electrographic camera images obtained duringsounding rocket flights in 1975 and 1982. The 1975 images were centeredclose to the belt of Orion while the 1982 images were centeredapproximately 9 deg further north. One hundred and fifty stars fell inthe overlapping region and were observed with both cameras. Sixty-eightpercent of the objects were tentatively identified with known starsusing the SIMBAD database while another 24% are blends of objects tooclose together to separate with our resolution. As in previous studies,the majority of the identified ultraviolet sources are early-type stars.However, there are a significant number for which no such identificationwas possible, and we suggest that these are interesting objects whichshould be further investigated. Seven stars were found which were brightin the ultraviolet but faint in the visible. We suggest that some ofthese are nearby white dwarfs.

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Osservazione e dati astrometrici

Costellazione:Orione
Ascensione retta:05h05m13.05s
Declinazione:+08°56'31.7"
Magnitudine apparente:7.444
Distanza:275.482 parsec
Moto proprio RA:2.2
Moto proprio Dec:-5.4
B-T magnitude:7.409
V-T magnitude:7.442

Cataloghi e designazioni:
Nomi esatti
HD 1989HD 32660
TYCHO-2 2000TYC 685-1003-1
USNO-A2.0USNO-A2 0975-01330185
HIPHIP 23666

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