The dust emissivity index β in infrared-bright galaxies at 1.5 < z < 4.2
Artikel i vetenskaplig tidskrift, 2025

We have measured the dust emissivity index for 21 infrared-bright sources (including several gravitationally lensed galaxies) at <![CDATA[$1.5 < z using Atacama Large Millimetre/submillimetre Array 101-199 GHz data sampling the Rayleigh-Jeans side of the spectral energy distribution. These data are largely insensitive to temperature variations and therefore should provide robust measurements of. We obtain a mean of 2.2 with a standard deviation of 0.6 that is at the high end of the range of values that had previously been measured in many galactic and extragalactic sources. We find no systematic variation in versus redshift. We also demonstrate with a subset of our sources that these higher values have significant implications for modelling dust emission and in particular for calculating dust masses or the wavelength at which dust becomes optically thick.

submillimetre: galaxies

galaxies: ISM

infrared: galaxies

galaxies: high-redshift

Författare

G. J. Bendo

University of Manchester

Tom Bakx

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik

H. Algera

National Astronomical Observatory of Japan

Hiroshima University

Academia Sinica

A. Amvrosiadis

Durham University

S. Berta

Institut de Radioastronomie Millimétrique (IRAM)

L. Bonavera

Instituto Universitario de Ciencias y Tecnologías Espaciales de Asturias (ICTEA)

Universidad de Oviedo

P. Cox

Institut d 'Astrophysique de Paris

G. De Zotti

Istituto nazionale di astrofisica (INAF)

S. Eales

Cardiff University

J. González-Nuevo

Instituto Universitario de Ciencias y Tecnologías Espaciales de Asturias (ICTEA)

Universidad de Oviedo

Masato Hagimoto

Nagoya University

D. Ismail

Observatoire Astronomique de Strasbourg

D. A. Riechers

Universität zu Köln

S. Serjeant

Open University

M. W.L. Smith

Cardiff University

P. Temi

National Aeronautics and Space Administration (NASA)

Takafumi Tsukui

Australian National University

S. Urquhart

Open University

C. Vlahakis

National Radio Astronomy Observatory

Monthly Notices of the Royal Astronomical Society

00358711 (ISSN) 13652966 (eISSN)

Vol. 540 2 1560-1577

Ämneskategorier (SSIF 2025)

Astronomi, astrofysik och kosmologi

DOI

10.1093/mnras/staf816

Mer information

Senast uppdaterat

2025-06-13