[PDF] Top 20 The helium burning evolution of low mass stars
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The helium burning evolution of low mass stars
... The more luminous Cepheids W vir star s are identified with stars undergoing blueward loops from the second giant branch in response to helium shell flashes or finally e volving to the b[r] ... See full document
162
Implications of the generation of internal gravity waves by penetrative convection for the internal rotation evolution of low-mass stars
... of stars and the seismic data provided by the space-borne missions CoRoT and Kepler turn out to be a goldmine of information for the stellar evolution the- ...of stars, made the measurement of the ... See full document
5
The EBLM Project V Physical properties of ten fully convective, very low mass stars
... ten stars, and exceeds the radius predicted by the Exeter/Lyon stellar evolution ...of mass and radius is shown in Figure ...stellar evolution models (Dotter et ...very-low-mass ... See full document
19
Low-Mass Stars and Their Companions
... young stars, we can measure their masses by observing the kinematics of the disk of gas and dust surrounding the star (Czekala et ...of stars with ages larger than 10 million years but not yet onto the main ... See full document
235
The secondary stars in cataclysmic variables and low-mass X-ray binaries
... the mass–radius diagram (but see Howell, Hauschildt & Dhillon ...secondary stars will be difficult to distinguish from late-type main-sequence ... See full document
15
A Search for Pulsation in Young Brown Dwarfs and Very Low Mass Stars
... Many very low mass young cluster members are now catalogued and thus available for time series monitoring. Nevertheless, there is a wide range in both the quality and quantity of data available on them. In ... See full document
317
Brown dwarf formation by binary disruption
... enough mass to reach the hydrogen-burning ...its mass is essentially con- ...sufficient mass to also spawn two or three other ...very low- mass prestellar cores. ... See full document
6
2D dynamics of the radiative core of low mass stars
... of low mass stars all along their evolution is of primary interest when studying their rotational dynamics, internal mixing and magnetic field ...type stars at different evolutionary ... See full document
5
Precision diagnostics of pulsation and evolution in helium rich low mass stars
... lead stars HE 2359–2844 and HE 1256–2738 are proto-subdwarfs, evolving onto the ex- tended horizontal ...and helium sinks out of the ...the helium-deficient subdwarfs. If the fraction of halo ... See full document
219
Simulating radio emission from low mass stars
... convective, low-mass stars is generated is far from complete; however, magnetic imaging of bright, rapidly rotating stars through Zeeman Doppler Imaging ( ZDI; Semel 1989; Donati et ...and ... See full document
8
Positive Impact Program Evaluation
... B stars; it is also where all nearby star forming regions are found: the Scorpius-Centaurus star forming region ( ∼ 100 pc away), on the other side of the sky, Taurus-Auriga ( ∼ 150 pc away), Perseus, and Orion ... See full document
372
The APACHE Project
... favorable mass ratios allow for detection of rocky, potentially habitable planets with the RV technique, thanks to the moderately large amplitudes of the RV signals (a few ...the mass range between Neptune ... See full document
8
Young, Low-Mass Stars: X-rays and Circumstellar Environments
... photodissociation is sufficiently large, the atmosphere can be pushed out of thermochemical equilib- rium (see, e.g., Moses, 2014; Miguel & Kaltenegger, 2014; Hu & Seager, 2014). This effect has been observed in ... See full document
248
Reaction rate for carbon burning in massive stars
... medium mass nuclei [19, 20], where it was ob- served that at low energies the fusion cross sections fall off faster than expected by coupled-channels (CC) calcula- tions using standard Woods-Saxon ...at ... See full document
6
Studies of low mass interacting binary stars
... The secondary component is also found to occupy an interesting position on the HR diagram, lying near the ZAMS line, to the left of the other B-type secondary com ponents, and to the right of the W -type secondary ... See full document
289
Probing the Milky Way
... Time Evolution of Thermal Jets Associated with Low Mass Young Stars is targeting these objects, with the aim of testing specific morphological predictions of jet ...from low-mass ... See full document
5
Low-mass stars: Open problems all along their evolution
... the evolution on the AGB differ significantly from author to author, as can easily be verified in the ...core mass at the first thermal pulse differs widely from those published in [24] for masses in the ... See full document
10
Observational probes of helium ignition in low mass stars
... the low–metallicity ...RGB stars older than 6 Gyr should be observed, in agreement with observations, but the high metallicity of stars from 6–12 Gyr is not well–fit by the simple ...metal–poor ... See full document
173
Selected topics in the evolution of low-mass stars
... inactive stars, and thus the established concrete possibility of guiding mechanical energy toward the acceleration zone of cool stellar winds along flux tubes [71], further exploration of the Cranmer & Saar ... See full document
11
Far infrared cavity of a post C-rich AGB star under IRAS survey
... He-core burning phase is about 10 times shorter than the H-core burning shell so that the He-core burning leaves a C/O core behind that is surrounded by both a hydrogen and helium ... See full document
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