Contingut
Imatges
Carregar la teva Imatge
DSS Images Other Images
Articles Relacionats
Photoelectric V and (B-V) for McCuskey stars near the Galactic anticenter V and (B-V) for 135 stars near the Galactic anticenter were obtained.The ultimate purpose of the study is to establish accurate colors which,in conjunction with DDO-derived spectral and luminosity classes, willenable interstellar absorption correction. Ninety-four of these starsalso have been observed by McCuskey for a stellar density analysis ofthe Galactic anticenter. The specific objective here is to establish therelationship between the presented photoelectric and McCuskey'sphotographic colors and magnitudes. Small but significant systematicdifferences exist between the two systems. These differences, ifuniversal for McCuskey's entire sample, increase his distances by about20 percent and decrease his densities by about 40 percent.
| The stellar distribution in the galactic anticenter. Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1967AJ.....72.1199M&db_key=AST
|
Enviar un nou article
Enllaços Relacionats
- - No s'ha trobat enllaços -
Enviar un nou enllaç
Membre dels grups següents:
|
Dades d'Observació i Astrometria
Constel·lació: | Taurus |
Ascensió Recta: | 05h55m23.36s |
Declinació: | +25°55'18.1" |
Magnitud Aparent: | 9.055 |
Moviment propi RA: | 4.7 |
Moviment propi Dec: | -26.9 |
B-T magnitude: | 10.714 |
V-T magnitude: | 9.192 |
Catàlegs i designacions:
|