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HD 41895


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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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Dades d'Observació i Astrometria

Constel·lació:Orion
Ascensió Recta:06h07m34.17s
Declinació:-03°36'12.1"
Magnitud Aparent:8.121
Distancia:2272.727 parsecs
Moviment propi RA:-5.1
Moviment propi Dec:-1.5
B-T magnitude:8.205
V-T magnitude:8.128

Catàlegs i designacions:
Noms Propis   (Edit)
HD 1989HD 41895
TYCHO-2 2000TYC 4787-1520-1
USNO-A2.0USNO-A2 0825-01950000
HIPHIP 29037

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