Results 1 to 10 of about 10,786,884 (386)

The Protostellar Luminosity Function [PDF]

open access: yesThe Astrophysical Journal, 2011
The protostellar luminosity function (PLF) is the present-day luminosity function of the protostars in a region of star formation. It is determined using the protostellar mass function (PMF) in combination with a stellar evolutionary model that provides ...
Andre   +43 more
core   +2 more sources

Quasar Luminosity Function at z = 7 [PDF]

open access: yesThe Astrophysical Journal Letters, 2023
We present the quasar luminosity function (LF) at z = 7, measured with 35 spectroscopically confirmed quasars at 6.55 < z < 7.15. The sample of 22 quasars from the Subaru High- z Exploration of Low-Luminosity Quasars (SHELLQs) project, combined with 13 ...
Yoshiki Matsuoka   +43 more
doaj   +2 more sources

A Left and Right Truncated Schechter Luminosity Function for Quasars

open access: yesGalaxies, 2017
The luminosity function for quasars (QSOs) is usually fitted by a Schechter function. The dependence of the number of quasars on the redshift, both in the low and high luminosity regions, requires the inclusion of a lower and upper boundary in the ...
Lorenzo Zaninetti
doaj   +4 more sources

The Luminosity Function of M3 [PDF]

open access: yesThe Astrophysical Journal, 1999
We present a high precision, large sample luminosity function (LF) for the Galactic globular cluster M3. With a combination of ground based and Hubble Space Telescope data we cover the entire radial extent of the cluster.
A. Chieffi   +27 more
core   +2 more sources

The PICS project: II. Circumnebular extinction variations and their effect on the planetary nebula luminosity function [PDF]

open access: goldFrontiers in Astronomy and Space Sciences
For decades, the theoretical understanding of planetary nebulae (PNe) has remained in tension with the observed universal bright-end cutoff of the PN luminosity function (PNLF).
Lucas M. Valenzuela   +5 more
doaj   +2 more sources

Characterizing the luminosity components of luminous infrared galaxies in multi-wavelength from the X-ray to the far-infrared [PDF]

open access: yesScientific Reports
We characterize luminosity components of Ultra/Luminous Infrared Galaxies (U/LIRGs) in multi-wavelength from the X-ray to far-infrared. A set of 63 AGN U/LIRGs was selected where these galaxies are powered by a central active galactic nucleus (AGN ...
Abdallah A. M. Ali   +3 more
doaj   +2 more sources

Shedding light on the galaxy luminosity function [PDF]

open access: yesAstronomy and Astrophysics Review, 2011
95 pages, 23 figures, 3 tables. Now published in The Astronomy & Astrophysics Review. This version: bring in line with A&AR format requirements, also minor typo corrections made, additional citations and higher rez images ...
exaly   +3 more sources

The Luminosity Function of Galaxies in Some Nearby Clusters

open access: yesUHD Journal of Science and Technology, 2021
In the present work, the galaxy luminosity function (LF) has been studied for a sample of seven clusters in the redshift range (0.0 ≲ z ≲ 0.1), within Abell radius (1.5 h−1 Mpc), in the five SDSS passbands ugriz.
Mariwan Ahmed Rasheed   +1 more
doaj   +1 more source

On the mass distribution of stars in the solar neighborhood [PDF]

open access: yesSerbian Astronomical Journal, 2006
The present authors analyze samples consisting of Hipparcos stars. Based on the corresponding HR diagrams they estimate masses of Main-Sequence stars from their visual magnitudes. They find that already beyond the heliocentric radius of 10 pc the effects
Ninković S., Trajkovska V.
doaj   +1 more source

Luminosity function of GRBs [PDF]

open access: yesAstronomy & Astrophysics, 2001
We attempt to constrain the luminosity function of Gamma Ray Bursts (GRBs) from the observed number count--flux relation and the afterglow redshift data. We assume three classes of luminosity functions for our analysis: (a) Log-normal distribution, (b) Schechter distribution, and (c) Scale-free distribution. We assume several models of the evolution of
Sethi, Shiv, Bhargavi, S. G.
openaire   +2 more sources

Home - About - Disclaimer - Privacy