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Table · dataset · 2026

JCMT SCUBA-2 obs. of M31 with Herschel & Planck data

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We have carried out unprecedentedly deep, nearly confusion-limited JCMT SCUBA-2 mapping observations on the nearest spiral galaxy, M31 (Andromeda).

Description

The 850{mu}m image with a ~50pc resolution yields a comprehensive catalog of 383 giant molecular clouds (GMCs) that are associated with the spiral arms. In addition, it unveiled a population of 189 compact interarm GMCs in M31, which are mostly unresolved or marginally resolved.

The masses of all these GMCs are in the range of 2x10^4^-6x10^6^M_{sun}_; the sizes are in the range of 30-130pc. They follow a mass-size correlation, M{propto}Rc^2.5^. The interarm GMCs are systematically less massive, more diffuse, colder, and have lower star formation efficiency (SFE) than on-arm GMCs.

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Moreover, within individual spatially resolved on-arm and off-arm M31 GMCs, the SFE is considerably lower than the SFE in molecular clouds in main-sequence and green valley galaxies. Follow-up investigations on M31 GMCs may provide clues for how star formation may be quenched in galactic environments. Finally, we reconstrained the dust opacity spectral index {beta} in the M31 galaxy by combining our new JCMT observations with archival Herschel and Planck data and found that the radial variation in {beta} may not be as large as has been proposed by previous studies.

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Stated by source
Millimeter · Radio
Inferred from text
Astronomical sciences 70% · Image 75%
Provenance · 1 source records, 11 field assertions
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