Results 131 to 140 of about 5,073 (240)

Asteroseismology of red giants [PDF]

open access: yes, 2014
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]

open access: yesSpace Sci Rev, 2023
Hotta H   +4 more
europepmc   +1 more source

Revisiting the Impact of Stellar Magnetic Activity on the Detectability of Solar-Like Oscillations by Kepler

open access: yesFrontiers in Astronomy and Space Sciences, 2019
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]

open access: bronze, 1993
R. W. Noyes   +4 more
openalex   +1 more source

The Prospects for Asteroseismology from Ground-based Sites [PDF]

open access: bronze, 1996
J. N. Heasley   +5 more
openalex   +1 more source

Asteroseismology of RXJ 2117+3412, the hottest pulsating PG 1159 star [PDF]

open access: bronze, 2002
G. Vauclair   +43 more
openalex   +3 more sources

Editorial: Asteroseismology in the Kepler Era

open access: yesFrontiers in Astronomy and Space Sciences, 2021
Anthony E. Lynas-Gray   +6 more
doaj   +1 more source

A small survey of UV-bright stars around the northern ecliptic pole: seeking new p-mode sdB variables for the TESS mission

open access: yesOpen Astronomy, 2019
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

open access: yesUniverse
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

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