Results 131 to 140 of about 5,486 (209)
, 1963 HD 49798 was found to be a hot subdwarf. It is, at the present time the brightest member of this group and also the only one known spectroscopic binary. The complete paper will appear in the "Publications of the Astronomical Society of the Pacific".
Jaschek, Mercedes, Jaschek, Carlos
openaire +1 more source
Photometric variability in four hot subdwarf stars [PDF]
, 2016 D. Kilkenny, C. Koen
openalex +1 more source
Globular clusters, Hipparcos, and the age of the galaxy. [PDF]
Proc Natl Acad Sci U S A, 1998 Reid N.
europepmc +1 more source
Models of very-low-mass stars, brown dwarfs and exoplanets. [PDF]
Philos Trans A Math Phys Eng Sci, 2012 Allard F, Homeier D, Freytag B.
europepmc +1 more source
The Evolution of Compact Binary Star Systems. [PDF]
Living Rev Relativ, 2014 Postnov KA, Yungelson LR.
europepmc +1 more source
The age of the universe. [PDF]
Proc Natl Acad Sci U S A, 1997 Spergel DN, Bolte M, Freedman W.
europepmc +1 more source
Post-main-sequence planetary system evolution. [PDF]
R Soc Open Sci, 2016 Veras D.
europepmc +1 more source