Results 41 to 50 of about 249,783 (233)

Discovery of four new EL CVn-type binaries in the Gaia eclipsing binaries [PDF]

open access: yes, 2023
In this paper, we performed a search for EL CVn-type binaries based on the Gaia and TESS data. Through the combination of the Gaia DR3 eclipsing binary catalogue and the Gaia DR3 spectroscopic binary catalogue, we have identified 13 stars exhibiting EL CVn-like characteristics.
arxiv   +1 more source

Multiplicity among solar-type stars IV. The CORAVEL radial velocities and the spectroscopic orbits of nearby K dwarfs [PDF]

open access: yesA&A 619, A81 (2018), 2018
Context. The statistical properties of binary stars are clues for understanding their formation process. A radial velocity survey was carried on amongst nearby G-type stars and the results were published in 1991. Aims. The survey of radial velocity measurements was extended towards K-type stars. Methods.
arxiv   +1 more source

Low Mass Ratio Contact Binary V410 Aur and V776 Cas - II [PDF]

open access: yesJournal of Astronomy and Space Sciences, 2005
New BVR CCD light curves of the low mass ratio contact binaries, V410 Aur and V776 Cas, were observed with the 61 cm reflector and a 2K CCD camera at the Sobaeksan Astronomical Observatory.
Kyu-Dong Oh, Chun-Hwey Kim, Ho-iL Kim
doaj   +1 more source

Orbital Solutions for Two Young, Low-Mass Spectroscopic Binaries in Ophiuchus [PDF]

open access: yes, 2010
We report the orbital parameters for ROXR1 14 and RX J1622.7-2325Nw, two young, low-mass, and double-lined spectroscopic binaries recently discovered in the Ophiuchus star forming region. Accurate orbital solutions were determined from over a dozen high-resolution spectra taken with the Keck II and Gemini South telescopes.
arxiv   +1 more source

The Poincaré Pear and Poincaré-Darwin Fission Theory in Astrophysics, 1885-1901

open access: yesPhilosophia Scientiæ, 2023
In the early 1880s, Henri Poincaré discovered an equilibrium figure for uniformly-rotating fluid masses—the pear, or piriform figure—and speculated that in certain circumstances the pear splits into two unequal parts, and provides thereby a model for the
Scott A. Walter
doaj   +1 more source

The Value-Added Catalog of ASAS-SN Eclipsing Binaries III: Masses and Radii of Gaia Spectroscopic Binaries [PDF]

open access: yes, 2022
Masses and radii of stars can be derived by combining eclipsing binary light curves with spectroscopic orbits. In our previous work, we modeled the All-Sky Automated Survey for Supernovae (ASAS-SN) light curves of more than 30,000 detached eclipsing binaries using PHOEBE.
arxiv   +1 more source

The VLT-FLAMES Tarantula Survey XXII. Multiplicity properties of the B-type stars [PDF]

open access: yes, 2015
We investigate the multiplicity properties of 408 B-type stars observed in the 30 Doradus region of the Large Magellanic Cloud with multi-epoch spectroscopy from the VLT-FLAMES Tarantula Survey (VFTS).
Apellániz, J. Maíz   +9 more
core   +3 more sources

A Radial Velocity Survey of the Cygnus OB2 Association [PDF]

open access: yes, 2006
We conducted a radial velocity survey of the Cygnus OB2 Association over a 6 year (1999 - 2005) time interval to search for massive close binaries. During this time we obtained 1139 spectra on 146 OB stars to measure mean systemic radial velocities and ...
Andy J. Monson   +28 more
core   +3 more sources

Mining Double-line Spectroscopic Candidates in the LAMOST Medium-resolution Spectroscopic Survey Using a Human–AI Hybrid Method

open access: yesThe Astrophysical Journal Supplement Series
We utilize a hybrid approach that integrates the traditional cross-correlation function (CCF) and machine learning to detect spectroscopic multiple star systems, specifically focusing on double-line spectroscopic binaries (SB2s).
Shan-shan Li   +7 more
doaj   +1 more source

Evidence of a Decreased Binary Fraction for Massive Stars within 20 milliparsecs of the Supermassive Black Hole at the Galactic Center

open access: yesThe Astrophysical Journal, 2023
We present the results of the first systematic search for spectroscopic binaries within the central 2 × 3 arcsec ^2 around the supermassive black hole at the center of the Milky Way galaxy.
Devin S. Chu   +14 more
doaj   +1 more source

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