Results 141 to 150 of about 169 (167)
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A luminosity function for star clusters in the Large Magellanic Cloud

Publications of the Astronomical Society of the Pacific, 1985
A luminosity function for star clusters brighter than MB = -4.5 in the LMC is determined from eye estimates of the integrated magnitudes of all clusters in two large regions of the LMC. The differential luminosity function rises monotonically toward faint magnitudes.
R. A. W. Elson, S. M. Fall
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The Bolometric Luminosity Function for the Lowest Mass Stars

1992
We present a luminosity function (LF) for the coolest stars in three POSSII fields — extending earlier LFs to much lower masses at higher precision than has been acheived previously.
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Luminosity and mass functions for low main-sequence stars

Astrophysics and Space Science, 1972
The luminosity function derived for main sequence stars in the neighbourhood of the Sun shows evidence for a flattening in the interval 5≲M v ≲8. An interpretation of this feature by means of theoretical models enables us to deduce the mass function for stars belonging to the main sequence.
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Luminosity function of stars

Astrophysics, 1977
R. A. Bartaya, E. K. Kharadze
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Liminosity distribution function for visual binary stars

Astrophysics and Space Science, 1985
The ‘cosmic scatter’ of 147 of the best known visual binary stars on the Main Sequence is discussed and a new estimation of the luminosity distribution function for multiple star systems is presented. As long as the mass ratio q of a close binary is not smaller than 0.5, the distribution of close binary components is identical to the van Rhijn ...
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Evolution of luminosity function of faint stars

Astrophysics, 1989
O. Yu. Malkov, A. �. Piskunov
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The Luminosity Function of Carbon Stars in the Large Magellanic Cloud

1981
The luminosity function of a complete sample of late type carbon stars in the LMC is compared with a luminosity function derived from recent evolutionary models. It appears from this comparison that present stellar evolutionary calculations of thermally pulsing asymptotic giant branch stars are inadequate to explain the bulk of the carbon stars.
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On the FRB luminosity function – – II. Event rate density

Monthly Notices of the Royal Astronomical Society, 2020
Wei-Yang Wang, Rui Luo
exaly  

The ALMA REBELS Survey: the first infrared luminosity function measurement at z  ∼ 7

Monthly Notices of the Royal Astronomical Society, 2023
Pascal Oesch   +2 more
exaly  

The Durham/UKST Galaxy Redshift Survey - II. The field galaxy luminosity function

Monthly Notices of the Royal Astronomical Society, 1998
Tom Shanks, R Fong, Q A Parker
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