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HD 43407


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Far-ultraviolet stellar photometry - A field in Monoceros
FUV photometry of stars in a field in Monoceros in the wavelength rangefrom 1230 to 1600 A has been carried out using data from anelectrographic Schmidt camera carried on a sounding rocket. Ultravioletmagnitudes were extracted for 602 objects in the field. Fifty-eightpercent were tentatively identified with visible stars using the SIMBADdata base while another 25 percent are blends of objects too closetogether to separate with our resolution. Eleven of the UV objectscoincide with parts of the star clusters NGC 2169, NGC 2244, and NGC2264 in which individual stars cannot be resolved. As in previousstudies, the majority of the identified ultraviolet sources areidentified with early-stars. However, there are a significant number forwhich no such identification was possible, and we suggest that many ofthese are nearby white dwarfs.

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Dades d'Observació i Astrometria

Constel·lació:Orion
Ascensió Recta:06h16m05.21s
Declinació:+03°05'50.8"
Magnitud Aparent:8.043
Distancia:165.563 parsecs
Moviment propi RA:3.3
Moviment propi Dec:-6.7
B-T magnitude:8.138
V-T magnitude:8.051

Catàlegs i designacions:
Noms Propis
HD 1989HD 43407
TYCHO-2 2000TYC 136-1671-1
USNO-A2.0USNO-A2 0900-02605940
HIPHIP 29766

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