The Transformation of a Main Sequence Star Into a Red-Giant Star in the Core-And-Shell Model

American Journal of Physics - United States
doi 10.1119/1.19456
Full Text
Abstract

Available in full text

Date
Authors
Publisher

American Association of Physics Teachers (AAPT)

Related search

Asteroseismic Measurement of Surface-To-Core Rotation in a Main-Sequence Star

EPJ Web of Conferences
AstronomyPhysics
2015English

Hydrodynamical Simulations of Turbulent Convection in a Rotating Red Giant Star

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2008English

Survival of a Brown Dwarf After Engulfment by a Red Giant Star

Nature
Multidisciplinary
2006English

Geometry of Giant Star Model Atmospheres: A Consistency Test

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2006English

HST GHRS Observations of the Herbig Ae Star HD104237: First UV Observations of a Hot Disk Wind From a Pre-Main Sequence Star

International Astronomical Union Colloquium
1997English

&Epsiv; Aurigæ—a Super-Giant Star

Nature
Multidisciplinary
1938English

Kinematic Distances of Pre-Main-Sequence Stars in the Lupus Star-Forming Region

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2012English

Detection of a Planetary Companion Around the Giant Star Γ1Leonis

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2010English

Star Formation History of a Young Super-Star Cluster in NGC 4038/39: Direct Detection of Low-Mass Pre-Main Sequence Stars

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2010English

Amanote Research

Note-taking for researchers

Follow Amanote

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

Privacy PolicyRefund Policy