output
20142024
most citedALMA-IMF I -- Investigating the origin of stellar masses: Introduction to the Large Program and first results

95 citations

9 papers

astro-ph.GA2024★ 1 cited

Accretion vs. Core-Filament Collision: Implications for Streamer Formation in Per-emb-2

Fumitaka Nakamura, Quang Nguyen-Luong, Kousuke Ishihara +1

Recent millimeter and submillimeter observations have unveiled elongated and asymmetric structures around protostars. These structures, referred to as streamers, often exhibit cohe…

astro-ph.GA2024

An ultra wide-band, high-sensitivity Q-band receiver for single-dish telescopes, eQ: rest frequency determination of CCS ( = -) and SO ( = -), and high-redshift CO ( = 1-0) detection

Fumitaka Nakamura, Chau-Ching Chiong, Kotomi Taniguchi +16

We report on the development and commissioning of a new Q-band receiver for the Nobeyama 45-m telescope, covering 30--50 GHz with a receiver noise temperature of about 15 K. We nam…

astro-ph.SR2023

NIKA2 observations of dust grain evolution from star-forming filament to T-Tauri disk: Preliminary results from NIKA2 observations of the Taurus B211/B213 filament

Q. Nguyen-Luong, R. Adam, P. Ade +51

To understand the evolution of dust properties in molecular clouds in the course of the star formation process, we constrain the changes in the dust emissivity index from star-form…

astro-ph.GA2022★ 9 cited

The SEDIGISM survey: Molecular cloud morphology. II. Integrated source properties

K. R. Neralwar, D. Colombo, A. Duarte-Cabral +21

The Structure, Excitation, and Dynamics of the Inner Galactic InterStellar Medium (SEDIGISM) survey has produced high (spatial and spectral) resolution CO (2-1) maps of the…

astro-ph.GA2022★ 17 cited

The SEDIGISM survey: Molecular cloud morphology. I. Classification and star formation

K. R. Neralwar, D. Colombo, A. Duarte-Cabral +22

We present one of the very first extensive classifications of a large sample of molecular clouds based on their morphology. This is achieved using a recently published catalogue of…

astro-ph.GA2021★ 95 cited

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

F. Motte, S. Bontemps, T. Csengeri +61

The ALMA-IMF Large Program imaged a total noncontiguous area of 53pc2, covering 15 extreme, nearby protoclusters of the Milky Way. They were selected to span relevant early protocl…