The Stellar Population in the rho Ophiuchi Cluster

1993 ◽  
Vol 416 ◽  
pp. 185 ◽  
Author(s):  
F. Comeron ◽  
G. H. Rieke ◽  
A. Burrows ◽  
M. J. Rieke
Keyword(s):  
Stellar Population ◽  
Rho Ophiuchi

Further mid-infrared study of the rho Ophiuchi cloud young stellar population: Luminosities and masses of pre-main-sequence stars

1994 ◽  
Vol 434 ◽  
pp. 614 ◽  
Author(s):  
Thomas P. Greene ◽  
Bruce A. Wilking ◽  
Philippe Andre ◽  
Erick T. Young ◽  
Charles J. Lada
Keyword(s):  
Stellar Population ◽  
Main Sequence ◽  
Main Sequence Stars ◽  
Infrared Study ◽  
Mid Infrared ◽  
Rho Ophiuchi

scholarly journals “The mass distribution of the young stellar population in Chamaeleon I and in Rho Ophiuchi”

1991 ◽  
Vol 147 ◽  
pp. 427-429
Author(s):  
Jane C. Gregório Hetem ◽  
J.R.D. Lépine ◽  
R. Ortiz
Keyword(s):  
Star Formation ◽  
Mass Distribution ◽  
Formation Process ◽  
Stellar Population ◽  
Age Distribution ◽  
Young Stars ◽  
Rho Ophiuchi ◽  
Hr Diagram

We obtain the mass distribution and the age distribution of the young stars associated with Chamaeleon I and Rho Ophiuchi, two nearby sites of star formation. Our method consists in determining the temperature and the luminosity of each object in order to locate it on the HR diagram, and then comparing the position on the HR diagram with the evolutionary tracks and isochrones presented by Cohen and Kuhi (1979). The star-formation process is found to have started more recently in ρ Oph than in Cham I.

The evolutionary status of the stellar population in the rho Ophiuchi cloud core

1995 ◽  
Vol 438 ◽  
pp. 813 ◽  
Author(s):  
Karen M. Strom ◽  
Jeremy Kepner ◽  
Stephen E. Strom
Keyword(s):  
Stellar Population ◽  
Evolutionary Status ◽  
Rho Ophiuchi ◽  
Cloud Core

scholarly journals “The mass distribution of the young stellar population in Chamaeleon I and in Rho Ophiuchi”

1991 ◽  
Vol 147 ◽  
pp. 427-429
Author(s):  
Jane C. Gregório Hetem ◽  
J.R.D. Lépine ◽  
R. Ortiz
Keyword(s):  
Star Formation ◽  
Mass Distribution ◽  
Formation Process ◽  
Stellar Population ◽  
Age Distribution ◽  
Young Stars ◽  
Rho Ophiuchi ◽  
Hr Diagram

We obtain the mass distribution and the age distribution of the young stars associated with Chamaeleon I and Rho Ophiuchi, two nearby sites of star formation. Our method consists in determining the temperature and the luminosity of each object in order to locate it on the HR diagram, and then comparing the position on the HR diagram with the evolutionary tracks and isochrones presented by Cohen and Kuhi (1979). The star-formation process is found to have started more recently in ρ Oph than in Cham I.

Statistical criteria of stellar population types

1966 ◽  
Vol 24 ◽  
pp. 101-110
Author(s):  
W. Iwanowska
Keyword(s):  
Stellar Population ◽  
Chemical Properties ◽  
Spectrophotometric Study ◽  
Physical And Chemical Properties ◽  
Population Type ◽  
The Galaxy ◽  
Distribution Parameters ◽  
Physical And Chemical ◽  
Statistical Criteria ◽  
And Chemical Properties

In connection with the spectrophotometric study of population-type characteristics of various kinds of stars, a statistical analysis of kinematical and distribution parameters of the same stars is performed at the Toruń Observatory. This has a twofold purpose: first, to provide a practical guide in selecting stars for observing programmes, second, to contribute to the understanding of relations existing between the physical and chemical properties of stars and their kinematics and distribution in the Galaxy.

Stellar Population Synthesis in AGN Host Galaxies

2001 ◽  
Vol 1 ◽  
pp. 145-152
Author(s):  
M. Joly ◽  
C. Boisson ◽  
J. Moultaka ◽  
D. Pelat
Keyword(s):  
Stellar Population ◽  
Population Synthesis ◽  
Host Galaxies ◽  
Stellar Population Synthesis

Infrared Studies of the Young Stellar Population of 30 Doradus

1980 ◽  
Vol 4 (1) ◽  
pp. 90-92
Author(s):  
P. J. McGregor ◽  
A. R. Hyland
Keyword(s):  
Star Formation ◽  
Stellar Population ◽  
Cluster Formation ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Formation Processes ◽  
Excellent Opportunity ◽  
Infrared Studies ◽  
30 Doradus

The 30 Doradus region offers an excellent opportunity to study cluster formation processes and recent star formation in the Large Magellanic Cloud.

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