Results 1 to 10 of about 550,992 (335)
Internal rotation of red giants by asteroseismology [PDF]
We present an asteroseismic approach to study the dynamics of the stellar interior in red giant stars by asteroseismic inversion of the splittings induced by the stellar rotation on the oscillation frequencies.
Christensen-Dalsgaard J. +14 more
doaj +11 more sources
Red giant seismology: Observations [PDF]
The CoRoT and Kepler missions provide us with thousands of red-giant light curves that allow a very precise asteroseismic study of these objects. Before CoRoT and Kepler, the red-giant oscillation patterns remained obscure.
Mosser B.
doaj +3 more sources
Livestock Grazing Management Influences Survival of Giant and Red Pandas in Southwest China [PDF]
Despite intensified global efforts in wildlife conservation, livestock grazing remained a critical factor driving habitat changes. The quantitative studies specifically addressing the impact of grazing on the habitat changes of giant (Ailuropoda ...
Yanshan Zhou +15 more
doaj +2 more sources
Rapidly rotating red giants [PDF]
Stellar oscillations give seismic information on the internal properties of stars. Red giants are targets of interest since they present mixed modes, wich behave as pressure modes in the convective envelope and as gravity modes in the radiative core ...
Gehan Charlotte +2 more
doaj +5 more sources
Theoretical Uncertainties in Red Giant Branch Evolution: The Red Giant Branch Bump [PDF]
A Monte Carlo simulation exploring uncertainties in standard stellar evolution theory on the red giant branch of metal-poor globular clusters has been conducted.
Alongi M. +11 more
core +6 more sources
Asteroseismology of red giants & galactic archaeology [PDF]
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 +4 more sources
AbstractTwo principal mechanisms that may be responsible for mass loss from red giants are considered: shock wave-driven winds and radiatively (dust)-driven winds. Effect of the periodic shocks accompanying nonlinear oscillations of red giants is most prominent in the outer layers of the stellar atmosphere where shocks are able not only to expel gas ...
Yu. A. Fadeyev
openalex +3 more sources
Probing the Deep End of the Milky Way with New Oscillating Kepler Giants [PDF]
The Kepler mission has been a success in both exoplanet search and stellar physics studies. Red giants have actually been quite a highlight in the Kepler scene.
Mathur Savita +7 more
doaj +2 more sources
Red-giant stars in eccentric binaries [PDF]
The unparalleled photometric data obtained by NASA’s Kepler Space Telescope has led to improved understanding of red-giant stars and binary stars. We discuss the characterization of known eccentric system, containing a solar-like oscillating red-giant ...
Beck P. G. +6 more
doaj +6 more sources
Red giant collisions in the Galactic Centre [PDF]
10 pages, 11 figures, MNRAS (in press)
Vernon C. Bailey, M. B. Davies
openalex +4 more sources

