Several post-common envelope binaries have slightly increasing, decreasing or oscillating orbital periods. One of several possible explanations is light travel-time changes, caused by the binary centre-of-mass being perturbed by the gravitational pull of
Bogensberger David +2 more
doaj +1 more source
Erratum: Radial velocity measurements of Subdwarf B stars: Table 1. [PDF]
C. M. Copperwheat +4 more
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Candidate subdwarfs and white dwarfs from the 2MASS, Tycho-2, XPM and UCAC3 catalogues [PDF]
George A. Gontcharov +3 more
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Distance and Age of M92 From Hipparcos Subdwarfs [PDF]
F. Pont +3 more
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On the Capability of Oxidovanadium(IV) Derivatives to Act as All-Around Catalytic Promoters Since the Prebiotic World. [PDF]
Campitelli P, Crucianelli M.
europepmc +1 more source
ORFEUS II echelle spectra: On the influence of iron-group line blanketing in the Far-UV spectral range of hot subdwarfs [PDF]
J. L. Deetjen
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Detection of Long‐Period Variations in the Subdwarf B Star PG 0101+039 on the Basis of Photometry from theMOSTSatellite [PDF]
S. K. Randall +13 more
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EVR-CB-004: An Inflated Hot Subdwarf O Star + Unseen WD Companion in a Compact Binary Discovered with the Evryscope [PDF]
Jeffrey K. Ratzloff +12 more
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Amplitude and frequency variations in PG~0101+039 from K2 photometry -- A pulsating hot B subdwarf star in an unsynchronized binary system [PDF]
Xiao-Yu Ma +5 more
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