Study of the region of star formation 2 Mon. The region of the cluster NGC 2244

Journal Article · Fri Nov 01 04:00:00 EST 1985 · Astrophysics (Engl. Transl.); (United States)

DOI:https://doi.org/10.1007/BF01029724· OSTI ID:5315277

Guseva, N G

This paper studies the distribution and density of the dust in the central part region of star formation 2 Mon in the young open star cluster NGC 2244. The ring of the cluster coincides with the ring emission of the Rosette nebula, and the nucleus of the cluster contains five O stars and is in the emission hole. On the basis of data from the author's catalog of B and V magnitudes and the spectra of O-B-A stars, and also data on UBV photometry and proper motions, it is concluded that there is no dust in the eastern half of the ring of maximal emission of the Rosette nebula.

• Research Organization: Principal Astronomical Observatory, Ukrainian Academy of Sciences
• OSTI ID: 5315277
• Journal Information: Astrophysics (Engl. Transl.); (United States), Journal Name: Astrophysics (Engl. Transl.); (United States) Vol. 22:3; ISSN ATPYA
• Country of Publication: United States
• Language: English

Related Subjects

640102* -- Astrophysics & Cosmology-- Stars & Quasi-Stellar
Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ABSORPTION SPECTRA
BRIGHTNESS
COLOR
COSMIC DUST
COSMIC GASES
COSMIC RADIO SOURCES
DIAGRAMS
DISTRIBUTION
DUSTS
EMISSION SPECTRA
FLUIDS
FUNCTIONS
GASES
H2 REGIONS
NEBULAE
OPACITY
OPTICAL DEPTH CURVE
OPTICAL PROPERTIES
ORGANOLEPTIC PROPERTIES
PHOTOMETRY
PHYSICAL PROPERTIES
SPATIAL DISTRIBUTION
SPECTRA
SPECTRAL DENSITY
SPECTRAL FUNCTIONS
STAR ACCRETION
STAR CLUSTERS
STAR EVOLUTION
STARS