Results 101 to 110 of about 43,328 (216)
Classifying Single Stars and Spectroscopic Binaries Using Optical Stellar Templates [PDF]
Benjamin R. Roulston+2 more
openalex +1 more source
Li-rich Unevolved Stars from LAMOST-MRS
Based on the spectra from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope medium-resolution spectroscopic survey, we select a sample of 88 Li-rich unevolved star candidates.
Ze-Ming Zhou+17 more
doaj +1 more source
The CHARA Catalog of Orbital Elements of Spectroscopic Binary Stars [PDF]
Stuart F. Taylor+2 more
openalex +1 more source
Spectroscopic search for binaries among EHB stars in globular clusters
To appear in Baltic Astronomy. Proceedings of the 2nd meeting on Hot Subdwarf Stars, La Palma, June 2005.
MONI BIDIN C+5 more
openaire +4 more sources
Polarimetric Variations of Binary Stars. V. Pre-Main-Sequence Spectroscopic Binaries Located in Ophiuchus and Scorpius [PDF]
N. Manset, Pierre Bastien
openalex +1 more source
NGC 2506 is a rich, intermediate-age (2.0 Gyr), metal-poor ([Fe/H] ∼ −0.2) open cluster. This work presents the results of 12,157 spectroscopic radial-velocity measurements of 2442 stars in the NGC 2506 field obtained over 41 yr, made as part of the WIYN
Evan Linck+2 more
doaj +1 more source
The Lower Main Sequence of Stars in the Solar Neighborhood: Model Predictions Versus Observation
We have used the Simbad database and VizieR catalogue access tools to construct the observational color-absolute magnitude diagrams of nearby K-M dwarfs with precise Hipparcos parallaxes (σπ/π ≤ 0:05).
Bartašiūtė S.+3 more
doaj +1 more source
11 pages, 2 figures; to be published in MNRAS; RV measurements and orbits will be distributed in the on-line SB9 catalogue. Revision 1: the on-line only material was added to the printed version; 1 ascii data file and 67 figures in eps ...
Halbwachs, Jean-Louis+2 more
openaire +2 more sources
We present the first estimate of the intrinsic binary fraction of young stars across the central ≈0.4 pc surrounding the supermassive black hole (SMBH) at the Milky Way Galactic center (GC).
Abhimat K. Gautam+10 more
doaj +1 more source
Recently, a double-lined binary classical Cepheid, OGLE-LMC-CEP-1347, was discovered with the orbital period ( P _orb = 59 days), 5 times shorter than that of any binary Cepheid known before.
Felipe Espinoza-Arancibia+1 more
doaj +1 more source