Results 111 to 120 of about 5,486 (209)
Aims. The formation mechanisms of spectrally diverse hot subdwarfs remain unclear. While existing mass distribution analyses suggest additional channels beyond helium white dwarf (He-WD) mergers contribute to He-rich subdwarf formation, these conclusions
Feng Mengqi +6 more
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News on the X-ray emission from hot subdwarf stars
In latest years, the high sensitivity of the instruments on-board the XMM-Newton and Chandra satellites allowed us to explore the properties of the X-ray emission from hot subdwarf stars.
Palombara Nicola La, Mereghetti Sandro
doaj +1 more source
Time resolved spectroscopy of the multiperiodic pulsating subdwarf B star PG 1605+072 [PDF]
A. Tillich
openalex +1 more source
Envelope loss of RGB/AGB stars and the formation of hot subdwarfs
Low mass stars may lose their envelopes in the first giant branch (RGB) or the asymptotic giant branch (AGB) via envelope ejection (i.e. superwind). The envelope loss of AGB stars leads to the formation of carbon-oxygen (CO) white dwarfs (WDs), while the
Chen X., Han Z.
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On the formation of single and binary helium-rich subdwarf O stars [PDF]
Stephen Justham +2 more
openalex +1 more source
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
openalex +1 more source
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
Discovery of [CLC][ITAL]p[/ITAL][/CLC]-Mode Instabilities in the Hot Subdwarf B Star PG 1047+003 [PDF]
M. Billères +6 more
openalex +1 more source
The first massive compact companion in a wide orbit around a hot subdwarf star [PDF]
S. Geier +7 more
openalex +1 more source
We design a convolutional neural network incorporating channel attention and spatial attention mechanisms to predict atmospheric parameters of hot subdwarfs.
Zhenxin Lei +6 more
doaj +1 more source

