Results 91 to 100 of about 199 (140)

A new hot subdwarf

, 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

The Evolution of Compact Binary Star Systems. [PDF]

Living Rev Relativ, 2014
Postnov KA, Yungelson LR.
europepmc   +1 more source

Globular cluster ages. [PDF]

Proc Natl Acad Sci U S A, 1998
Jimenez R.
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

The stars of low luminosity. [PDF]

Proc Natl Acad Sci U S A, 1974
Luyten WJ.
europepmc   +1 more source

Classification of LAMOST spectra of B-type and hot subdwarf stars using kernel support vector machine. [PDF]

Sci Rep
Tahir M, Yude B, Mehmood T, Bashir S, Zhenping Y, Awais M.   +5 more
europepmc   +1 more source

Galaxies and large scale structure at high redshifts. [PDF]

Proc Natl Acad Sci U S A, 1998
Steidel CC.
europepmc   +1 more source

Old disk subdwarfs

The Astrophysical Journal, 1978
J. R. Mould, D. B. McElroy
openaire   +1 more source

Performance of an automated computerized plate scanner. [PDF]

Proc Natl Acad Sci U S A, 1971
Luyten WJ.
europepmc   +1 more source