Hi-GAL, the Herschel infrared Galactic Plane Survey: photometric maps and compact source catalogues-First data release for the inner Milky Way:+ 68°≥ l≥− 70°

S Molinari, E Schisano, D Elia, M Pestalozzi… - Astronomy & …, 2016 - aanda.org
Aims. We present the first public release of high-quality data products (DR1) from Hi-GAL,
the Herschel infrared Galactic Plane Survey. Hi-GAL is the keystone of a suite of continuum …

Cloud–cloud collisions and triggered star formation

Y Fukui, A Habe, T Inoue, R Enokiya… - Publications of the …, 2021 - ieeexplore.ieee.org
Star formation is a fundamental process for galactic evolution. One issue over the last
several decades has been determining whether star formation is induced by external …

Clouds, filaments, and protostars: the herschel Hi-GAL milky way

S Molinari, B Swinyard, J Bally, M Barlow… - Astronomy & …, 2010 - aanda.org
We present the first results from the science demonstration phase for the Hi-GAL survey, the
Herschel key program that will map the inner Galactic plane of the Milky Way in 5 bands. We …

The Hi-GAL compact source catalogue – I. The physical properties of the clumps in the inner Galaxy (−710 < ℓ < 670)

D Elia, S Molinari, E Schisano… - Monthly Notices of …, 2017 - academic.oup.com
Abstract Hi-GAL (Herschel InfraRed Galactic Plane Survey) is a large-scale survey of the
Galactic plane, performed with Herschel in five infrared continuum bands between 70 and …

Ammonia from cold high-mass clumps discovered in the inner Galactic disk by the ATLASGAL survey

M Wienen, F Wyrowski, F Schuller, KM Menten… - Astronomy & …, 2012 - aanda.org
Context. The APEX Telescope Large Area Survey: the GALaxy (ATLASGAL) is an unbiased
continuum survey of the inner Galactic disk at 870 μm. It covers±60° in Galactic longitude …

ALMA-IMF-VI. Investigating the origin of stellar masses: Core mass function evolution in the W43-MM2&MM3 mini-starburst

Y Pouteau, F Motte, T Nony, M González… - Astronomy & …, 2023 - aanda.org
Context. Among the most central open questions regarding the initial mass function (IMF) of
stars is the impact of environment on the shape of the core mass function (CMF) and thus …

FEEDBACK: A SOFIA legacy program to study stellar feedback in regions of massive star formation

N Schneider, R Simon, C Guevara… - Publications of the …, 2020 - iopscience.iop.org
FEEDBACK is a SOFIA (Stratospheric Observatory for Infrared Astronomy) legacy program
dedicated to study the interaction of massive stars with their environment. It performs a …

Characterizing precursors to stellar clusters with Herschel

C Battersby, J Bally, A Ginsburg, JP Bernard… - Astronomy & …, 2011 - aanda.org
Context. Despite their profound effect on the universe, the formation of massive stars and
stellar clusters remains elusive. Recent advances in observing facilities and computing …

[图书][B] Molecular astrophysics

AGGM Tielens - 2021 - books.google.com
Focusing on the organic inventory of regions of star and planet formation in the interstellar
medium of galaxies, this comprehensive overview of the molecular universe is an invaluable …

The Bolocam Galactic Plane Survey. XIV. Physical Properties of Massive Starless and Star-forming Clumps

BE Svoboda, YL Shirley, C Battersby… - The Astrophysical …, 2016 - iopscience.iop.org
We sort 4683 molecular clouds between 10< ℓ< 65 from the Bolocam Galactic Plane Survey
based on observational diagnostics of star formation activity: compact 70 μm sources, mid-IR …