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Carbon star
Evolution, Mass Loss and Variability of Low and Intermediate-Mass Stars What Are Low and Intermediate Mass Stars?
The Deaths of Stars
U Antliae — a Dying Carbon Star
Stellar Spectral Classification of Previously Unclassified Stars Gsc 4461-698 and Gsc 4466-870" (2012)
Carbon Stars T. Lloyd Evans
Stellar Evolution
198 4Apj. . .211 . .7 91N the Astrophysical Journal, 277:791-805
GEORGE HERBIG and Early Stellar Evolution
PREFACE Symposium 177 of the International Astronomical Union
Late Stages of Stellar Evolution*
William Pendry Bidelman (1918-2011)
CGCS 673 Is a Semi-Regular Variable Carbon Star, Study Finds 23 June 2020, by Tomasz Nowakowski
A Binary-Induced Pinwheel Outflow from the Extreme Carbon Star, AFGL 3068
Studying Asymptotic Giant Branch Stars in the JWST Era
Stellar Evolution on the Asymptotic Giant Branch: Some Actualities
Search for Wolf-Rayet, Carbon and M Stars in External Galaxies with the GRISM/GRENS Technique J
Dust Production Around Carbon-Rich Stars: the Role of Metallicity
Mira Variables Explained by a Planetary Companion Interaction: a Means to Drop the Pulsation Paradigm?
Top View
The Unusual Spitzer Spectrum of the Carbon Star Iras 04496А6958
Observing Stellar Evolution
Chapter 17--Star Stuff
The Chemical Composition of Carbon Stars. the R-Type Stars
Physical Properties of Stars and Stellar Dynamics
Is There a Metallicity Ceiling to Form Carbon Stars? – a Novel Technique Reveals a Scarcity of C-Stars in the Inner M31 Disk⋆ M
Carbon Star Wind Models at Solar and Sub-Solar Metallicities: a Comparative Study I
The Hidden Transition from AGB to Post-AGB Stars As Observed by AKARI
Asteroseismology
Carbon Star Observing Program
Carbon Star CGCS 673 Identified As a Semi-Regular Variable Star
A Chandra Study: Are Dwarf Carbon Stars Spun up and Rejuvenated by Mass Transfer?
The Effective Temperatures of Carbon-Rich Stars
Tour the Sky's Reddest Stars
Evolution of Asymptotic Giant Branch Stars I
Advances in Spectral Classification
Asymptotic Giant Branch Stars Viewed Up-Close and Far-Off
Understanding AGB Carbon Star Nucleosynthesis from Observations