Results 81 to 90 of about 199 (140)

From synthetic SEDs to stellar origins: A deep learning model for physical parameter retrieval in hot subdwarf stars

open access: yesAstronomy & Astrophysics
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
doaj   +1 more source

Some Subdwarf Models

open access: yes, 1962
In this paper we present the results obtained from the numerical integration of the equations for the case of subdwarfs with masses comparable and somewhat larger than that of the Sun.
Varsavsky, Carlos Manuel   +2 more
openaire   +1 more source

Subdwarfs. II - The missing halo-population K subdwarfs

open access: yesThe Astrophysical Journal, 1979
M. S. Bessell, D. T. Wickramasinghe
openaire   +1 more source

On the Colors of Subdwarfs.

open access: yesThe Astrophysical Journal, 1955
M. Schwarzschild, L. Searle, R. Howard
openaire   +1 more source

Deep Learning–driven Atmospheric Parameter Prediction for Hot Subdwarf Stars with Synthetic and Observed Spectra

open access: yesThe Astrophysical Journal Supplement Series
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

Models of very-low-mass stars, brown dwarfs and exoplanets. [PDF]

open access: yesPhilos Trans A Math Phys Eng Sci, 2012
Allard F, Homeier D, Freytag B.
europepmc   +1 more source

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