ALMA observations of α Centauri - First detection of main-sequence stars at 3 mm wavelength

2014/12/10 by R. Liseau, W. H. T. Vlemmings, W. Vlemmings +29 · 3 citations
Physics and Astronomy · #Astro and Planetary Science #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Chromosphere #Context (archaeology) #Galaxy #Globular cluster #Main sequence #Millimeter #Physics #Radiative transfer #Solar and Space Plasma Dynamics #Spectral line #Stars #Stellar, planetary, and galactic studies #Wavelength #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201425189

published as A&A 573, L4 (2015) · 5 pages, 3 figures, Letter to Astronomy and Astrophysics

arxiv created 2014/12/12 · arxiv updated 2014/12/24 · openalex publication_date 2015/01/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/04

Abstract

Astronomy and Astrophysics 573 (2015): L4 reproduced with permission from Astronomy & Astrophysics, © ESO

Citations

• The Ups and Downs of Alpha Centauri
• DUst around NEarby Stars. The survey observational results
• How dusty is alpha Centauri? Excess or non-excess over the infrared photospheres of main-sequence stars

Cited by

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