Results 41 to 50 of about 12,099 (232)
T35: A Small Automatic Telescope for Long‐Term Observing Campaigns
The T35 is a small telescope (14″) equipped with a large format CCD camera installed in the Sierra Nevada Observatory (SNO) in Southern Spain. This telescope will be a useful tool for the detecting and the studying of pulsating stars, particularly, in open clusters.
Susana Martín-Ruiz +11 more
wiley +1 more source
The Structure and Evolution of Stars: Introductory Remarks
In this introductory chapter of the Special Issue entitled ‘The Structure and Evolution of Stars’, we highlight the recent major progress made in our understanding of the physics that governs stellar interiors.
Dominic M. Bowman +2 more
doaj +1 more source
The Quest for Pulsating M Dwarf Stars
Recent fully non-adiabatic theoretical studies of M dwarf models show that they have the potential to excite radial, and low-order, low-degree non-radial modes, as well as solar-like oscillations, due to models being completely convective or having large
Cristina Rodríguez-López
doaj +1 more source
Asteroseismology of Close Binary Stars: Tides and Mass Transfer
The study of stellar oscillations allows us to infer the properties of stellar interiors. Meanwhile, fundamental parameters such as mass and radius can be obtained by studying stars in binary systems. The synergy between binarity and asteroseismology can
Zhao Guo
doaj +1 more source
Towards gravitational wave asteroseismology [PDF]
11 pages, 8 figures, mn ...
Andersson, Nils, Kokkotas, Kostas D.
openaire +4 more sources
Asteroseismology of red giants & galactic archaeology
Red-giant stars are low- to intermediate-mass ($M \lesssim 10$~M$_{\odot}$) stars that have exhausted hydrogen in the core. These extended, cool and hence red stars are key targets for stellar evolution studies as well as galactic studies for several ...
A. Baglin +72 more
core +1 more source
Pulsation in Intermediate-Mass Stars
A new perspective of pulsation in stars within the δ Scuti instability strip has recently emerged as a result of Kepler observations. The majority of stars within the instability strip do not pulsate and practically all δ Scuti stars contain low ...
Luis A. Balona
doaj +1 more source
TESS asteroseismology of the known red-giant host stars HD 212771 and HD 203949 [PDF]
International ...
Adibekyan, Vardan +47 more
core +5 more sources
CoRoT and Kepler results: Solar-like oscillators
The space-borne observatories CoRoT (Convection Rotation and planetary Transits) and Kepler have provided photometric time series data of unprecedented precision for large numbers of stars.
Hekker, S.
core +1 more source
Helio- and asteroseismology [PDF]
AbstractObservations of solar and stellar oscillations are providing detailed information about stellar interiors. In the case of the Sun the set of observed frequencies is sufficiently detailed and accurate that the properties of the solar interior, such as sound speed, density and internal rotation, can be inferred with substantial precision and ...
openaire +3 more sources

