Corrigendum: Non-Vestoid candidate asteroids in the inner main belt (Astronomy and Astrophysics (2017) 599 (A107) DOI: 10.1051/0004-6361/201629551)

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[31] Corrigendum: ALMA spectral line and imaging survey of a low and a high mass-loss rate AGB star between 335 and 362 GHz( Astronomy and Astrophysics (2018) 615 (A28 )DOI: 10.1051/0004-6361/201732216)
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[32] Erratum: Herschel-planck dust optical-depth and column-density maps (Corrigendum): I. Method description and results for orion (Astronomy and Astrophysics (2014) A45 (566) DOI: 10.1051/0004-6361/201323293)
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[33] Corrigendum: A discontinuity in the luminosity mass relation and fluctuations in the evolutionary tracks of low-mass and low-metallicity stars at the Gaia M-dwarf gap (Astronomy and Astrophysics (2021) 650 (184) DOI: 10.1051/0004-6361/202140536)
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[34] Corrigendum: H I filaments are cold and associated with dark molecular gas HI4PI-based estimates of the local diffuse CO–dark H2 distribution (Astronomy and Astrophysics (2020) 639 (A26) DOI: 10.1051/0004-6361/202037602)
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[35] Erratum: Non-thermal desorption of complex organic molecules: Efficient CH3OH and CH3COOCH3sputtering by cosmic rays (Astronomy & Astrophysics (2019) 627 (A55) DOI: 10.1051/0004-6361/201834787)
Institut des Sciences Moléculaires dOrsay , UMR8214, Cnrs, Université de Paris-Sud, Université Paris-Saclay, Bât 520, Rue André Rivière, Orsay
91405, France
不详
91406, France
不详
14000, France
不详
91405, France
不详
110016, India
Astron. Astrophys., 2019,

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