Results 21 to 30 of about 152,062 (293)

The Eclipsing Binaries from the LAMOST Medium-resolution Survey. III. A High-precision Empirical Stellar Mass Library

open access: yesThe Astronomical Journal, 2023
High-precision stellar masses and radii measured directly from binaries can effectively calibrate stellar models. However, such a database containing full spectral types and a large range of metallicity is still not fully established. A continuous effort
Jianping Xiong   +8 more
doaj   +1 more source

Stellar Populations and Hubble Type [PDF]

open access: yesHighlights of Astronomy, 1983
Men are more apt to be mistaken in their generalization than in their particular observations. MachiavelliIt was already realized by Hubble (1936) that galaxy morphology and stellar content were correlated. He pointed out that resolution into stars increases along the classification sequence Sa-Sb-Sc.
openaire   +1 more source

Mixed Types of Stellar Populations [PDF]

open access: yesNature, 1948
ONE of the most interesting and most mysterious features of the stellar contents of our own and other known galaxies is the fact that there seem to exist two rather distinct types of stellar populations differing between themselves by mechanical as well as by physical properties of individual members.
openaire   +1 more source

Zeta-Payne: A Fully Automated Spectrum Analysis Algorithm for the Milky Way Mapper Program of the SDSS-V Survey

open access: yesThe Astronomical Journal, 2022
The Sloan Digital Sky Survey (SDSS) has recently initiated its fifth survey generation (SDSS-V), with a central focus on stellar spectroscopy. In particular, SDSS-V's Milky Way Mapper program will deliver multiepoch optical and near-infrared spectra for ...
Ilya Straumit   +15 more
doaj   +1 more source

New X-ray Selected Pre-Main Sequence Members of the Serpens Molecular Cloud [PDF]

open access: yes, 2013
The study of young stars no longer surrounded by disks can greatly add to our understanding of how protoplanetary disks evolve and planets form. We have used VLT/FLAMES optical spectroscopy to confirm the youth and membership of 19 new young diskless ...
Brown, Joanna M.   +2 more
core   +2 more sources

Stellar Populations in Field Early-Type Galaxies

open access: yesAstronomical Society of the Pacific Conference Series, 2007
We have acquired intermediate resolution spectra in the 3700-7000 A wavelength range for a sample of 65 early-type galaxies predominantly located in low density environments, a large fraction of which show emission lines. The spectral coverage and the high quality of the spectra allowed us to derive Lick line-strength indices and to study their ...
Annibali, F.   +4 more
openaire   +3 more sources

A Transparent Window into Early-type Stellar Variability

open access: yesThe Astrophysical Journal, 2022
Abstract Subsurface convection zones are ubiquitous in early-type stars. Driven by narrow opacity peaks, these thin convective regions transport little heat but play an important role in setting the magnetic properties and surface variability of stars.
Adam S. Jermyn   +2 more
openaire   +2 more sources

Revealing dark matter dress of primordial black holes by cosmological lensing

open access: yesPhysics Letters B, 2023
Stellar-mass primordial black holes (PBHs) from the early Universe can directly contribute to the gravitational wave (GW) events observed by LIGO, but can only comprise a subdominant component of the dark matter (DM).
Masamune Oguri   +2 more
doaj   +1 more source

Stellar populations of ultraluminous infrared galaxies

open access: yes, 2011
Ultraluminous infrared galaxies (ULIRGs) have several types according to dominance of starburst or AGN component. We made stellar population analysis for a sample of 160 ULIRGs to study the evolution of ULIRGs. We found that the dominance of intermediate-
Abazajian   +37 more
core   +1 more source

The Galaxy Population of Abell 1367: The Stellar Mass-Metallicity Relation

open access: yes, 2011
Using wide baseline broad-band photometry, we analyse the stellar population properties of a sample of 72 galaxies, spanning a wide range of stellar masses and morphological types, in the nearby spiral-rich and dynamically young galaxy cluster Abell 1367.
Balogh   +84 more
core   +1 more source

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