Amanote Research

Amanote Research

    RegisterSign In

White Dwarf Atmosphere Models With Ly-Alpha Opacity in the Analysis of the White Dwarf Cooling Sequence of NGC 6397

Astronomy and Astrophysics - France
doi 10.1051/0004-6361:20077985
Full Text
Open PDF
Abstract

Available in full text

Categories
AstrophysicsAstronomyPlanetary ScienceSpace
Date

September 4, 2007

Authors
P. M. Kowalski
Publisher

EDP Sciences


Related search

The White Dwarf Cooling Sequence in the Old Open Cluster NGC 188

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2002English

The White Dwarf Cooling Age of the Open Cluster NGC 2420

Astronomical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2000English

On the White Dwarf Cooling Sequence With Extremely Large Telescopes

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2013English

Cataclysmic Variables and a Candidate Helium White Dwarf in the Globular Cluster NGC 6397

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
1999English

White Dwarf Cooling Sequences

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2007English

A White Dwarf With an Oxygen Atmosphere

Science
MultidisciplinaryPhilosophy of ScienceHistory
2016English

Seismology of a Massive Pulsating Hydrogen Atmosphere White Dwarf

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2012English

Nucleosynthesis in White Dwarf Atmospheres.

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
1974English

Analysis of Pulsating White Dwarf Star Light Curves

2019English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2026 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy