Results 71 to 80 of about 2,116 (204)

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

The imprint of star formation on stellar pulsations. [PDF]

open access: yesNat Commun, 2022
Steindl T, Zwintz K, Vorobyov E.
europepmc   +1 more source

Precise determination of stellar parameters of the ZZ Ceti and DAZ white dwarf GD 133 through asteroseismology [PDF]

open access: green, 2019
J-N Fu   +17 more
openalex   +1 more source

Asteroseismology

open access: yes
21 pages; This is a pre-print of an invited chapter for the Encyclopedia of Astrophysics (edited by I. Mandel, section editor F.R.N.
Bowman, Dominic M., Bugnet, Lisa
openaire   +2 more sources

The ET mission to search for earth 2.0s. [PDF]

open access: yesInnovation (Camb), 2022
Ge J   +4 more
europepmc   +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

Gravitational-wave Asteroseismology with f-modes from Neutron Star Binaries at the Merger Phase [PDF]

open access: bronze, 2021
Harry Ho-Yin Ng   +3 more
openalex   +1 more source

Influence of Magnetic Activity on the Determination of Stellar Parameters Through Asteroseismology

open access: yesFrontiers in Astronomy and Space Sciences, 2019
Magnetic activity changes the gravito-acoustic modes of solar-like stars and in particular their frequencies. There is an angular-degree dependence that is believed to be caused by the non-spherical nature of the magnetic activity in the stellar ...
Fernando Pérez Hernández   +8 more
doaj   +1 more source

CCD Asteroseismology of Open Clusters [PDF]

open access: bronze, 1993
I. Vidal, Juan Antonio Belmonte
openalex   +1 more source

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