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 …

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 …

[HTML][HTML] Chasing discs around O-type (proto) stars: Evidence from ALMA observations

R Cesaroni, Á Sánchez-Monge, MT Beltrán… - Astronomy & …, 2017 - aanda.org
Context. Circumstellar discs around massive stars could mediate the accretion onto the star
from the infalling envelope, and could minimize the effects of radiation pressure. Despite …

ATLASGAL-selected massive clumps in the inner Galaxy-III. Dust continuum characterization of an evolutionary sample

C König, JS Urquhart, T Csengeri, S Leurini… - Astronomy & …, 2017 - aanda.org
Context. Massive-star formation and the processes involved are still poorly understood. The
ATLASGAL survey provides an ideal basis for detailed studies of large numbers of massive …

Two mass distributions in the L 1641 molecular clouds: the Herschel connection of dense cores and filaments in Orion A

D Polychroni, E Schisano, D Elia, A Roy… - The Astrophysical …, 2013 - iopscience.iop.org
We present Herschel survey maps of the L 1641 molecular clouds in Orion A. We extracted
both the filaments and dense cores in the region. We identified which of the dense sources …

The identification of filaments on far-infrared and submillimiter images: Morphology, physical conditions and relation with star formation of filamentary structure

E Schisano, KLJ Rygl, S Molinari… - The Astrophysical …, 2014 - iopscience.iop.org
Observations of molecular clouds reveal a complex structure, with gas and dust often
arranged in filamentary, rather than spherical geometries. The association of pre-and proto …

The first hi-gal observations of the outer galaxy: A look at star formation in the third galactic quadrant in the longitude range 216.° 5≲ ℓ≲ 225.° 5

D Elia, S Molinari, Y Fukui, E Schisano… - The Astrophysical …, 2013 - iopscience.iop.org
We present the first Herschel PACS and SPIRE photometric observations in a portion of the
outer Galaxy (216 fdg 5≲ ℓ≲ 225 fdg 5 and− 2≲ b≲ 0) as a part of the Hi-GAL survey. The …

ALMA-IMF-XII. Point-process mapping of 15 massive protoclusters

P Dell'Ova, F Motte, A Gusdorf, Y Pouteau… - Astronomy & …, 2024 - aanda.org
Context. A crucial aspect in addressing the challenge of measuring the core mass function
(CMF), that is pivotal for comprehending the origin of the initial mass function (IMF), lies in …

Far-Infrared Dust Temperatures and Column Densities of the MALT90 Molecular Clump Sample

AE Guzmán, P Sanhueza, Y Contreras… - The Astrophysical …, 2015 - iopscience.iop.org
We present dust column densities and dust temperatures for∼ 3000 young, high-mass
molecular clumps from the Millimeter Astronomy Legacy Team 90 GHz survey, derived from …