Carbon Chemistry in the Envelope of Vy Canis Majoris: Implications for Oxygen-Rich Evolved Stars

Astrophysical Journal - United States
doi 10.1088/0004-637x/695/2/1604
Full Text
Abstract

Available in full text

Date
Authors
Publisher

IOP Publishing

Related search

Aluminium Oxide in the Optical Spectrum of VY Canis Majoris

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2012English

Pure Rotational Spectra of TiO and TiO2in VY Canis Majoris

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2013English

Β Canis Majoris Stars in the (Β, [C1]) Plane

Symposium - International Astronomical Union
1974English

Submillimeter Vibrationally Excited Water Emission From the Peculiar Red Supergiant VY Canis Majoris

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2006English

ALMA Observations of Anisotropic Dust Mass Loss in the Inner Circumstellar Environment of the Red Supergiant VY Canis Majoris

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2014English

The Production of Low Mass Carbon Stars; Carbon-Rich Dredge Up or Oxygen-Rich Mass Loss?

International Astronomical Union Colloquium
1989English

A Spectrographic Study of [Beta] Canis Majoris

Lick Observatory Bulletins
1918English

The Effective Temperatures of Carbon-Rich Stars

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2001English

Full Evolutionary Models for PG 1159 Stars. Implications for the Helium-Rich O(He) Stars

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2006English

Amanote Research

Note-taking for researchers

Follow Amanote

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

Privacy PolicyRefund Policy