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Astronomy & Astrophysics

Volume 662 (June 2022)


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Letters to the Editor

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Linking stellar populations to H II regions across nearby galaxies - I. Constraining pre-supernova feedback from young clusters in NGC 1672 L6

DOI: https://doi.org/10.1051/0004-6361/202243766

Astrophysical processes

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Evidence for γ-ray emission from the remnant of Kepler’s supernova based on deep H.E.S.S. observations A65

DOI: https://doi.org/10.1051/0004-6361/202243096

Cosmology (including clusters of galaxies)

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Systematic errors on optical-SED stellar-mass estimates for galaxies across cosmic time and their impact on cosmology A86

DOI: https://doi.org/10.1051/0004-6361/202142577

Extragalactic astronomy

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Probing star formation and ISM properties using galaxy disk inclination - III. Evolution in dust opacity and clumpiness between redshift 0.0 < z < 0.7 constrained from UV to NIR A26

DOI: https://doi.org/10.1051/0004-6361/202142452
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The Fornax Deep Survey with the VST - XII. Low surface brightness dwarf galaxies in the Fornax cluster A43

DOI: https://doi.org/10.1051/0004-6361/202141756
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The dark matter halo masses of elliptical galaxies as a function of observationally robust quantities A55

DOI: https://doi.org/10.1051/0004-6361/202142511
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Physics of ULIRGs with MUSE and ALMA: The PUMA project - III. Incidence and properties of ionised gas disks in ULIRGs, associated velocity dispersion, and its dependence on starburstiness A94

DOI: https://doi.org/10.1051/0004-6361/202142659
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The LOFAR Two-metre Sky Survey Deep fields - The mass dependence of the far-infrared radio correlation at 150 MHz using deblended Herschel fluxes A100

DOI: https://doi.org/10.1051/0004-6361/202141307

Galactic structure, stellar clusters and populations

Interstellar and circumstellar matter

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ALMA-IMF - I. Investigating the origin of stellar masses: Introduction to the Large Program and first results A8

DOI: https://doi.org/10.1051/0004-6361/202141677
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The EDIBLES survey - V. Line profile variations in the λλ5797, 6379, and 6614 diffuse interstellar bands as a tool to constrain carrier sizes A24

DOI: https://doi.org/10.1051/0004-6361/202142225
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Gas phase Elemental abundances in Molecular cloudS (GEMS) - VI. A sulphur journey across star-forming regions: study of thioformaldehyde emission A52

DOI: https://doi.org/10.1051/0004-6361/202142936
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Importance of source structure on complex organics emission - I. Observations of CH3OH from low-mass to high-mass protostars A67

DOI: https://doi.org/10.1051/0004-6361/202142769
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CRIRES high-resolution near-infrared spectroscopy of diffuse interstellar band profiles - Detection of 12 new DIBs in the YJ band and the introduction of a combined ISM sight line and stellar analysis approach A81

DOI: https://doi.org/10.1051/0004-6361/202142990
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Observational constraints on gas disc sizes in the protoplanetary discs of multiple systems in the Taurus region A121

DOI: https://doi.org/10.1051/0004-6361/202141035

Stellar structure and evolution

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Erratum

The iron and oxygen content of LMC Classical Cepheids and its implications for the extragalactic distance scale and Hubble constant - Equivalent width analysis with Kurucz stellar atmosphere models (Corrigendum) C1

DOI: https://doi.org/10.1051/0004-6361/202142441e

Stellar atmospheres

The Sun and the Heliosphere

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Evidence of a complex structure within the 2013 August 19 coronal mass ejection - Radial and longitudinal evolution in the inner heliosphere A45

DOI: https://doi.org/10.1051/0004-6361/202142966

Planets and planetary systems

Atomic, molecular, and nuclear data

Astronomical instrumentation

Catalogs and data

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ALMA-IMF - II. Investigating the origin of stellar masses: Continuum images and data processing A9

DOI: https://doi.org/10.1051/0004-6361/202141681
Open Access

Stellar labels for hot stars from low-resolution spectra - I. The HotPayne method and results for 330 000 stars from LAMOST DR6 A66

DOI: https://doi.org/10.1051/0004-6361/202141570

Numerical methods and codes

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