Results 61 to 70 of about 19,129 (209)
Detection of Four Intermediate-mass Stars with Cool Companions in Low Mass Ratio Eclipsing Binaries
According to the core fragmentation and dynamical capture theories of binary formation, binaries tend to form with nearly equal masses. The detection of intermediate-mass binaries with low mass ratios challenges these theories, as such binaries may form ...
Linfeng Chang +3 more
doaj +1 more source
Abundance analysis of SB2 binary stars with HgMn primaries [PDF]
T. Ryabchikova
openalex +1 more source
Orbital Modulation Induced by a Third Component in the Overcontact Binary V0554 Dra
We present the first comprehensive photometric and spectroscopic analysis of the overcontact eclipsing binary V0554 Dra. By simultaneously modeling multiband light curves and radial velocity data using the Wilson–Devinney code, we determine that the ...
Mu-Lan Deng +10 more
doaj +1 more source
TYC 3340-2437-1: A Quadruple System with a Massive Star
Hierarchical massive quadruple systems are ideal laboratories for examining the theories of star formation, dynamical evolution, and stellar evolution.
Jiao Li +13 more
doaj +1 more source
Induced differential rotation and mixing in asynchronous binary stars [PDF]
Gloria Koenigsberger +2 more
openalex +1 more source
ICCD Speckle Observations of Binary Stars. XIX. An Astrometric/Spectroscopic Survey of O Stars [PDF]
Brian D. Mason +5 more
openalex +1 more source
The Binary Fraction of B-type Runaway Stars from LAMOST DR8
Runaway stars are defined as stars that depart from their birth clusters at high peculiar velocities. There are two main mechanisms for the formation of runaway stars, i.e., the binary-supernova scenario (BSS) and the dynamical ejection scenario (DES ...
Kun Chen +4 more
doaj +1 more source
CY Ari and IK Lyn are two eclipsing binary systems that share the same spectral type but exhibit significantly different metallicities. Based on the Wilson–Devinney (W-D) method, the first photometric solutions are obtained by analyzing the new complete ...
Hu-Shan Xu +5 more
doaj +1 more source
Short term variability in Be stars and binaries in the Magellanic Clouds [PDF]
Christophe Martayan +3 more
openalex +1 more source
Individual stars located near the caustics of galaxy clusters can undergo extreme magnification when crossing microcaustics, rendering them observable even at cosmological distances. Though most massive stars are likely to reside in binary systems rather
Wenwen Zheng +7 more
doaj +1 more source

