O-Star Mass-Loss Rates at Low Metallicity

Astronomy and Astrophysics - France
doi 10.1051/0004-6361/201219439
Full Text
Abstract

Available in full text

Date
Authors
Publisher

EDP Sciences

Related search

Neutron Nucleosynthesis in a Low-Mass, Low-Metallicity AGB Star

International Astronomical Union Colloquium
1989English

The Impact of Metallicity-Dependent Mass-Loss Versus Dynamical Heating on the Early Evolution of Star Clusters

Monthly Notices of the Royal Astronomical Society
AstrophysicsAstronomyPlanetary ScienceSpace
2014English

Massive Stars at Low Metallicity

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2013English

Neglecting the Porosity of Hot-Star Winds Can Lead to Underestimating Mass-Loss Rates

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2007English

Comparison of S-Processing Occurring in a Low Mass AGB Star of Low Metallicity and the Results of S-Classical Analysis

International Astronomical Union Colloquium
1989English

Low-Redshift Lowest-Metallicity Star-Forming Galaxies in the SDSS DR14

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2019English

Measuring Mass Loss Rates From Galactic Satellites

International Astronomical Union Colloquium
1999English

LSD and AMAZE: The Mass-Metallicity Relation at Z > 3

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2008English

STELLAR MASS–GAS-PHASE METALLICITY RELATION AT 0.5 ≤z≤ 0.7: A POWER LAW WITH INCREASING SCATTER TOWARD THE LOW-MASS REGIME

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2016English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2024 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy