Results 131 to 140 of about 5,073 (240)
Asteroseismology of red giants [PDF]
This chapter has been prepared for publication in "Asteroseismology", Canary Islands Winter School of Astrophysics, Volume XXII, edited by Pere L.
openaire +3 more sources
Dynamics of Large-Scale Solar Flows. [PDF]
Hotta H+4 more
europepmc +1 more source
Over 2,000 stars were observed for 1 month with a high enough cadence in order to look for acoustic modes during the survey phase of the Kepler mission. Solar-like oscillations have been detected in about 540 stars.
Savita Mathur+10 more
doaj +1 more source
The AFOE—A New Instrument for Asteroseismology [PDF]
R. W. Noyes+4 more
openalex +1 more source
The Prospects for Asteroseismology from Ground-based Sites [PDF]
J. N. Heasley+5 more
openalex +1 more source
Asteroseismology of RXJ 2117+3412, the hottest pulsating PG 1159 star [PDF]
G. Vauclair+43 more
openalex +3 more sources
Editorial: Asteroseismology in the Kepler Era
Anthony E. Lynas-Gray+6 more
doaj +1 more source
Starting in 2019, the TESS mission will monitor the northern ecliptic pole for 1 year. Data will be collected at 30-minute and 2-minute cadences, and only a limited amount of slots will be reserved for targets requiring a 20- second cadence.
Prins Saskia+2 more
doaj +1 more source
Magnetar QPOs and Neutron Star Crust Elasticity
The crust region is a tiny fraction of neutron stars, but it has a variety of physical properties and plays an important role in astronomical observations. One of the properties characterizing the crust is elasticity. In this review, with the approach of
Hajime Sotani
doaj +1 more source