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- W2000477519 abstract "view Abstract Citations (32) References (28) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The Luminosity Functions of Embedded Stellar Clusters. II. Numerical Results Fletcher, Andre B. ; Stahler, Steven W. Abstract We use the theory developed previously to calculate the evolving luminosity functions of very young stellar clusters. The luminosity function of the protostars alone quickly attains a characteristic, sharply peaked shape, which it maintains throughout the time of cluster formation. For the pre-main-sequence stars, the function continually changes but displays a pronounced 'step' near a luminosity of 10 Solar luminosity for a prolonged period. At most times, the vast majority of cluster members are pre-main-sequence stars. However, the total cluster luminosity is dominated first by the protostellar and later by the main-sequence component. At these late times, it is the brightest stars which reach the main sequence first. Finaly, a preliminary application of our model to the rho Ophiuchi embedded cluster indicates that star formation has proceeded in that region for 1 x 106. Publication: The Astrophysical Journal Pub Date: November 1994 DOI: 10.1086/174816 Bibcode: 1994ApJ...435..329F Keywords: Functions (Mathematics); Pre-Main Sequence Stars; Star Clusters; Stellar Evolution; Stellar Luminosity; Stellar Mass; Stellar Models; Mathematical Models; Ophiuchi Clouds; Star Formation; Astrophysics; STARS: EVOLUTION; STARS: LUMINOSITY FUNCTION; MASS FUNCTION; STARS: PRE--MAIN-SEQUENCE full text sources ADS | data products SIMBAD (7) Related Materials (1) Part 1: 1994ApJ...435..313F" @default.
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- W2000477519 title "The luminosity functions of embedded stellar clusters. 2: Numerical results" @default.
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