Quantitative spectroscopy of Deneb

2007/12/01 by F. Schiller, Florian Schiller, Norbert Przybilla +1 · 2 citations
Physics and Astronomy · #Astronomical spectroscopy #Astronomy and Astrophysical Research #Blue supergiant #COSMIC cancer database #Molecular spectroscopy #Scale (ratio) #Scientific Research and Discoveries #Spectroscopy #Stellar, planetary, and galactic studies #Supergiant #astro-ph

paper · pdf · doi:10.1051/0004-6361:20078590

17 pages, 12 figures. Accepted for publication in A&A

arxiv created 2007/12/01 · openalex publication_date 2008/01/02 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context.Quantitative spectroscopy of luminous BA-type supergiants offers a high potential for modern astrophysics. Detailed studies allow the evolution of massive stars, galactochemical evolution, and the cosmic distance scale to be constrained observationally.

Citations

• A New Extragalactic Distance Determination Method Using the Flux-weighted Gravity of Late B and Early A Supergiants
• Presupernova Evolution of Rotating Massive Stars. II. Evolution of the Surface Properties
• Presupernova Evolution of Differentially Rotating Massive Stars Including Magnetic Fields
• The Two Micron All Sky Survey (2MASS)
• Stellar evolution with rotation

Cited by

• Resolving the dusty circumstellar environment of the A[e] supergiant HD 62623 with the VLTI/MIDI
• Quantitative Spectroscopy of 24 A Supergiants in the Sculptor Galaxy NGC 300: Flux‐weighted Gravity–Luminosity Relationship, Metallicity, and Metallicity Gradient

Related

• Quantitative Spectroscopy of Supernovae for Dark Energy Studies
• Extragalactic Stellar Astronomy with Blue Supergiants
• Time, spatial, and spectral resolution of the Hαline-formation region of Deneb and Rigel with the VEGA/CHARA interferometer
• On the evolutionary nature of massive B-type supergiants: a modern empirical reappraisal using data from IACOB, Gaia and TESS
• Multi-component absorption lines in theHSTspectra of α Scorpii B