Results 221 to 230 of about 28,422 (257)
Some of the next articles are maybe not open access.
The Fermat star of binary trees
Information Processing Letters, 2009zbMATH Open Web Interface contents unavailable due to conflicting licenses.
LUCCIO, FABRIZIO, PAGLI, LINDA
openaire +3 more sources
Science, 1984
Most stars in the solar neighborhood are either double or multiple systems. They provide a unique opportunity to measure stellar masses and radii and to study many interesting and important phenomena. The best candidates for black holes are compact massive components of two x-ray binaries: Cygnus X-1 and LMC X-3.
openaire +2 more sources
Most stars in the solar neighborhood are either double or multiple systems. They provide a unique opportunity to measure stellar masses and radii and to study many interesting and important phenomena. The best candidates for black holes are compact massive components of two x-ray binaries: Cygnus X-1 and LMC X-3.
openaire +2 more sources
Astrophysics and Space Science, 2005
A brief review of Be stars in binaries is presented. Attention is paid to systems, where the Be phenomenon is clearly connected to the duplicity, but is not a simple consequence of mass transfer.
openaire +1 more source
A brief review of Be stars in binaries is presented. Attention is paid to systems, where the Be phenomenon is clearly connected to the duplicity, but is not a simple consequence of mass transfer.
openaire +1 more source
Binary and Multiple Star Formation
Astrophysics and Space Science, 1994From the growing observational evidence that binary/multiple star formation occurs prior to the pre-main sequence (Mathieu, 1992), it is clear that any theory of star formation MUST also explain binary formation. This paper details two formation mechanisms for binary/multiple stars, which occur simultaneously with protostar formation.
J. A. Turner +4 more
openaire +1 more source
Standard stars for binary-star interferometry
Publications of the Astronomical Society of the Pacific, 1983The authors present a list of 26 binary-star systems and propose that they be adopted as standards by all interferometric observers of binary stars. This will permit the discovery and elimination of systematic effects among observers and will also provide a readily available means of calibration.
H. A. McAlister, W. I. Hartkopf
openaire +1 more source
1996
Introduction Distinguishing neutron stars and black holes Optical companions and dynamical masses X-ray signatures of the nature of a compact object Structure and evolution of black-hole binaries High-mass black-hole binaries Low-mass black-hole binaries Low-mass black holes Formation of black holes in binaries Conclusions and future prospects.
openaire +2 more sources
Introduction Distinguishing neutron stars and black holes Optical companions and dynamical masses X-ray signatures of the nature of a compact object Structure and evolution of black-hole binaries High-mass black-hole binaries Low-mass black-hole binaries Low-mass black holes Formation of black holes in binaries Conclusions and future prospects.
openaire +2 more sources
Merger and Postmerger of Binary Neutron Stars with a Quark-Hadron Crossover Equation of State
Physical Review Letters, 2022Yong-Jia Huang +2 more
exaly