High-mass star and massive cluster formation in the milky way

F Motte, S Bontemps, F Louvet - Annual Review of Astronomy …, 2018 - annualreviews.org
This review examines the state-of-the-art knowledge of high-mass star and massive cluster
formation, gained from ambitious observational surveys, which acknowledges the multiscale …

On the application of machine learning in astronomy and astrophysics: A text‐mining‐based scientometric analysis

JV Rodríguez, I Rodríguez‐Rodríguez… - … Reviews: Data Mining …, 2022 - Wiley Online Library
Since the beginning of the 21st century, the fields of astronomy and astrophysics have
experienced significant growth at observational and computational levels, leading to the …

ATLASGAL–properties of a complete sample of Galactic clumps

JS Urquhart, C König, A Giannetti… - Monthly Notices of …, 2018 - academic.oup.com
Abstract The APEX Telescope Large Area Survey of the Galaxy (ATLASGAL) is an unbiased
870 μm submillimetre survey of the inner Galactic plane (| ℓ|< 60° with| b|< 1 5). It is the …

Unifying low-and high-mass star formation through density-amplified hubs of filaments-The highest mass stars (> 100 M⊙) form only in hubs

MSN Kumar, P Palmeirim, D Arzoumanian… - Astronomy & …, 2020 - aanda.org
Context. Star formation takes place in giant molecular clouds, resulting in mass-segregated
young stellar clusters composed of Sun-like stars, brown dwarfs, and massive O-type (50 …

ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions–XV. Steady accretion from global collapse to core feeding in massive hub-filament …

FW Xu, K Wang, T Liu, PF Goldsmith… - Monthly Notices of …, 2023 - academic.oup.com
ABSTRACT We present ALMA Band-3/7 observations towards 'the Heart'of a massive hub-
filament system (HFS) SDC335, to investigate its fragmentation and accretion. At a …

The Hi-GAL compact source catalogue–II. The 360° catalogue of clump physical properties

D Elia, M Merello, S Molinari, E Schisano… - Monthly Notices of …, 2021 - academic.oup.com
We present the 360° catalogue of physical properties of Hi-GAL compact sources, detected
between 70 and 500 m. This release not only completes the analogous catalogue previously …

The Star Formation Rate of the Milky Way as Seen by Herschel

D Elia, S Molinari, E Schisano, JD Soler… - The Astrophysical …, 2022 - iopscience.iop.org
We present a new derivation of the Milky Way's current star formation rate (SFR) based on
the data of the Herschel InfraRed Galactic Plane Survey (Hi-GAL). We estimate the …

ATLASGAL–evolutionary trends in high-mass star formation

JS Urquhart, MRA Wells, T Pillai… - Monthly Notices of …, 2022 - academic.oup.com
ABSTRACT ATLASGAL is an 870-µm dust survey of 420 deg2 the inner Galactic plane and
has been used to identify∼ 10 000 dense molecular clumps. Dedicated follow-up …

Protoplanetary disk birth in massive star-forming clumps: The essential role of the magnetic field

U Lebreuilly, P Hennebelle, T Colman… - The Astrophysical …, 2021 - iopscience.iop.org
Protoplanetary Disk Birth in Massive Star-forming Clumps: The Essential Role of the
Magnetic Field - IOPscience This site uses cookies. By continuing to use this site you agree …

N-bearing complex organics toward high-mass protostars-Constant ratios pointing to formation in similar pre-stellar conditions across a large mass range

P Nazari, JD Meijerhof, ML van Gelder… - Astronomy & …, 2022 - aanda.org
Context. Complex organic species are known to be abundant toward low-and high-mass
protostars. No statistical study of these species toward a large sample of high-mass …