Titlebook: New Quests in Stellar Astrophysics: The Link Between Stars and Cosmology; Proceedings of the I Miguel Chávez,Alessandro Bressan,Divakara Ma

LUCY

The Evolutionary Properties of Zero Metal Stars in the Mass Range between 4 and 100 M⊙In this review we will discuss the main evolutionary properties of the zero metallicity stars in the mass interval which extends from the intermediate mass to the massive stars together with their final yields.

演讲

Amenable

Grievance

Heating the Quiet Corona by Explosive Events in UV: Results from “Sumer” on Board Sohoure. We identified the times when the flux of a line attained the 3 and 5-σ levels. Moreover a considerably number of the events attained first a flux of 3 and 5-σ levels at a temperature of 1.5 10. K. We interpret the above results as an indication that most of the EE could be originated in the intermediate layers of the TR.

molest

A Grid of LTE Zero-Metallicity Stellar Fluxesce gravity. The coarse coverage in wavelength makes the grid suitable for continuum studies since the Lyman and Balmer breaks at 912 and 3647 Å respectively are among the most prominent features for the parameter space covered by the grid.

轻浮女

Conference proceedings 2002ehensive articles by leaders in fields extending from stellar atmospheres through properties of the stellar component in the Milky Way up to the stellar environment in high redshift galaxies...The wide coverage of astrophysical themes makes this volume very valuable for researchers and Ph.D. students in astrophysics. .

alcohol-abuse

SHRIK

Cool Stellar Atmosphereserved features of a given star with a single model atmosphere, however, a number of problems remain unsolved and will have to be addressed in the future, in particular for very low mass stars and substellar objects.

Debate

CORE