ALMA Reveals Diverse Dust-to-gas Mass Ratios and Quenching Modes in Old Quiescent Galaxies

Journal:

The Astrophysical Journal Letters

Published:

2025-12-16

DOI:

10.3847/2041-8213/ae226c

Affiliations:

23

Authors:

21

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Institutions	Authors	Share
National Centre for Nuclear Research (NCBJ), Poland	4.000000	0.19
Centre of Astrobiology (CAB), CSIC-INTA, Spain	2.000000	0.10
The University of British Columbia (UBC), Canada	1.000000	0.05
University of Massachusetts Amherst (UMass Amherst), United States of America (USA)	1.000000	0.05
University of Bologna (UNIBO), Italy	1.000000	0.05
Purple Mountain Observatory (PMO), CAS, China	1.000000	0.05
Technical University of Denmark (DTU), Denmark	1.000000	0.05
University of Padova (UNIPD), Italy	1.000000	0.05
Saint Mary's University (SMU), Canada	1.000000	0.05
Institute of Astrophysics and Space Sciences (IA), Portugal	1.000000	0.05
University of Cambridge, United Kingdom (UK)	1.000000	0.05
Scuola Internazionale Superiore di Studi Avanzati (SISSA), Italy	0.500000	0.02
Max Planck Institute for Radio Astronomy (MPIFR), Germany	0.500000	0.02
INAF - Astronomical Observatory of Padova (OAPD), Italy	0.500000	0.02
University of Florida (UF), United States of America (USA)	0.500000	0.02
Cosmic Dawn Center (DAWN), Denmark	0.500000	0.02
University of Washington (UW), United States of America (USA)	0.500000	0.02
The University of Texas at Austin (UT Austin), United States of America (USA)	0.500000	0.02
INAF - Osservatorio Astronomico d'Abruzzo, Italy	0.500000	0.02
Institute of Astrophysics of Canarias (IAC), Spain	0.500000	0.02
University of La Laguna (ULL), Spain	0.500000	0.02
Royal Observatory Edinburgh (ROE), United Kingdom (UK)	0.500000	0.02
University of the Western Cape (UWC), South Africa	0.500000	0.02

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