Results 121 to 128 of about 188,912 (128)

Spiral defect chaos with intermittency increases mean termination time. [PDF]

Phys Rev E
Mulimani MK, Rappel WJ.
europepmc   +1 more source

Some of the next articles are maybe not open access.

Related searches:

Bayesian sampling with BeAtlas, a grid of synthetic Be star spectra I. Recovering the fundamental parameters of α Eri and β CMi

Monthly notices of the Royal Astronomical Society, 2023
Classical Be stars are fast rotating, near main sequence B-type stars. The rotation and the presence of circumstellar discs profoundly modify the observables of active Be stars.
A. Rubio, A. Carciofi, P. Ticiani, B. Mota, R. G. Vieira, D. Faes, M. Genaro, T. H. de Amorim, R. Klement, I. Araya, C. Arcos, M. Curé, A. D. de Souza, C. Georgy, C. E. Jones, M. Suffak, A. C. F. Silva   +16 more
semanticscholar   +1 more source

Fundamental parameters for 30 faint open clusters with Gaia EDR3 based on the more reliable members

Nippon Tenmon Gakkai obun kenkyu hokoku, 2021
An open cluster is an ideal region to study the evolution of stars. In this work, we use Gaia Early Data Release 3 (Gaia EDR3) to derive the fundamental parameters of 30 faint open clusters listed in the catalogue given by Cantat-Gaudin et al. (2018, A&
Xu Ding, K. Ji, Xuzhi Li, Qiyuan Cheng, JinLiang Wang, Xiao-Guang Yu, Hui Liu   +6 more
semanticscholar   +1 more source

Relations between the asteroseismic indices and stellar parameters of δ Scuti stars for two years of TESS mission

, 2021
We investigate the relationship between the asteroseismic indices and the physical quantities of 438 δ Scuti (DSCT) stars observed by the Transiting Exoplanet Survey Satellite (TESS) mission at 26 sectors.
A. Hasanzadeh, H. Safari, H. Ghasemi
semanticscholar   +1 more source

Asteroseismic Determination of sdB Stars Fundamental Parameters

, 2004
S. Charpinet, P. Brassard, G. Fontaine
semanticscholar   +1 more source