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ALMA Lensing Cluster Survey: Deep 1.2 mm Number Counts and Infrared Luminosity Functions at z ≃ 1–8
DOI: 10.3847/1538-4365/ad5ae2 Bibcode: 2024ApJS..275...36F

Ouchi, Masami; Ivison, R. J.; Koekemoer, Anton M. +40 more

We present a statistical study of 180 dust continuum sources identified in 33 massive cluster fields by the Atacama Large Millimeter/submillimeter Array Lensing Cluster Survey (ALCS) over a total of 133 arcmin2 area, homogeneously observed at 1.2 mm. ALCS enables us to detect extremely faint millimeter sources by lensing magnification, …

2024 The Astrophysical Journal Supplement Series
Herschel eHST 53
The ALMA Survey of Star Formation and Evolution in Massive Protoclusters with Blue Profiles (ASSEMBLE): Core Growth, Cluster Contraction, and Primordial Mass Segregation
DOI: 10.3847/1538-4365/acfee5 Bibcode: 2024ApJS..270....9X

Ristorcelli, I.; Sanhueza, Patricio; Lee, Chang Won +40 more

The Atacama Large Millimeter/submillimeter Array (ALMA) Survey of Star Formation and Evolution in Massive Protoclusters with Blue Profiles (ASSEMBLE) aims to investigate the process of mass assembly and its connection to high-mass star formation theories in protoclusters in a dynamic view. We observed 11 massive (M clump ≳ 103

2024 The Astrophysical Journal Supplement Series
Herschel 28
A λ 3 mm Line Survey toward the Circumstellar Envelope of the Carbon-rich AGB Star IRC+10216 (CW Leo)
DOI: 10.3847/1538-4365/ad2460 Bibcode: 2024ApJS..271...45T

Zhang, Yong; Zhou, Jianjun; Szczerba, Ryszard +14 more

We present an unbiased λ 3 mm spectral line survey (between 84.5 and 115.8 GHz), conducted by the Purple Mountain Observatory 13.7 m radio telescope, together with updated modeling results, toward the carbon-rich asymptotic giant branch star IRC+10216 (CW Leo). A total of 75 spectral lines (96 transitions) are detected, and identified to arise fro…

2024 The Astrophysical Journal Supplement Series
Herschel 4
Mass-loss Rate of Highly Evolved Stars in the Magellanic Clouds
DOI: 10.3847/1538-4365/ad7b33 Bibcode: 2024ApJS..275...33W

Yang, Ming; Gao, Jian; Ren, Yi +3 more

Asymptotic giant branch stars (AGBs) and red supergiant stars (RSGs) exhibit significant mass-loss phenomena and are considered important sources of interstellar dust. In this work, we employed a uniform method of spectral energy distribution fitting to analyze a large, and hence statistically significant, sample of approximately 40,000 RSGs and A…

2024 The Astrophysical Journal Supplement Series
AKARI Gaia Herschel 1
Coevolution of Giant Molecular Clouds, Filaments, and Clumps as a Function of the Dense Gas Mass Fraction
DOI: 10.3847/1538-4365/ad7828 Bibcode: 2024ApJS..275....7Z

Li, Dalei; Tang, Xindi; Zhou, Jianjun +12 more

We investigate the evolutionary dynamics with archival continuum and line data of 27 giant molecular clouds (GMCs) in the Milky Way, focusing on their influence on star formation. Examining the dense gas mass fraction (DGMF) among the GMCs, we categorize them into low-DGMF (DGMF < 20%), medium-DGMF (20% < DGMF < 60%), and high-DGMF (60% &…

2024 The Astrophysical Journal Supplement Series
Herschel 1