PDRs4All: A JWST early release science program on radiative feedback from massive stars
The James Webb Space Telescope (JWST, Gardner et al. 2006) is a 6.5 m space telescope
launched in 2021 December and is developed by the National Aeronautics and Space …
launched in 2021 December and is developed by the National Aeronautics and Space …
FOREST unbiased Galactic plane imaging survey with the Nobeyama 45 m telescope (FUGIN). I. Project overview and initial results
T Umemoto, T Minamidani, N Kuno… - Publications of the …, 2017 - academic.oup.com
The FUGIN project is one of legacy projects using a new multi-beam FOREST (four-beam
receiver system on the 45 m telescope). This project aims to simultaneously investigate the …
receiver system on the 45 m telescope). This project aims to simultaneously investigate the …
The Hi-GAL compact source catalogue–II. The 360° catalogue of clump physical properties
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 …
between 70 and 500 m. This release not only completes the analogous catalogue previously …
Stellar feedback and triggered star formation in the prototypical bubble RCW 120
M Luisi, LD Anderson, N Schneider, R Simon… - Science …, 2021 - science.org
Radiative and mechanical feedback of massive stars regulates star formation and galaxy
evolution. Positive feedback triggers the creation of new stars by collecting dense shells of …
evolution. Positive feedback triggers the creation of new stars by collecting dense shells of …
Filament coalescence and hub structure in Mon R2-Implications for massive star and cluster formation
MSN Kumar, D Arzoumanian, A Men'Shchikov… - Astronomy & …, 2022 - aanda.org
There is growing evidence of the role of hub-filament systems (HFS) in the formation of stars
from low to high masses. As of today, however, the detailed structures of these systems are …
from low to high masses. As of today, however, the detailed structures of these systems are …
Self-absorption in [C II], 12CO, and HI in RCW120-Building up a geometrical and physical model of the region
S Kabanovic, N Schneider, V Ossenkopf-Okada… - Astronomy & …, 2022 - aanda.org
Aims. Revealing the 3D dynamics of H II region bubbles and their associated molecular
clouds and HI envelopes is important for develo** an understanding of the longstanding …
clouds and HI envelopes is important for develo** an understanding of the longstanding …
Globules and pillars in Cygnus XI. Herschel far-infrared imaging of the Cygnus OB2 environment
N Schneider, S Bontemps, F Motte, A Blazere… - Astronomy & …, 2016 - aanda.org
The radiative feedback of massive stars on molecular clouds creates pillars, globules and
other features at the interface between the H II region and molecular cloud. Optical and near …
other features at the interface between the H II region and molecular cloud. Optical and near …
COMAP Early Science. VI. A First Look at the COMAP Galactic Plane Survey
TJ Rennie, SE Harper, C Dickinson… - The Astrophysical …, 2022 - iopscience.iop.org
We present early results from the CO Map** Array Project (COMAP) Galactic Plane
Survey conducted between 2019 June and 2021 April, spanning 20< ℓ< 40 in Galactic …
Survey conducted between 2019 June and 2021 April, spanning 20< ℓ< 40 in Galactic …
THE ORION H ii REGION AND THE ORION BAR IN THE MID-INFRARED
We present mid-infrared photometry of the Orion bar obtained with the Faint Object infraRed
Camera for the SOFIA Telescope (FORCAST) on board SOFIA at 6.4, 6.6, 7.7, 19.7, 31.5 …
Camera for the SOFIA Telescope (FORCAST) on board SOFIA at 6.4, 6.6, 7.7, 19.7, 31.5 …
Ionization compression impact on dense gas distribution and star formation-Probability density functions around H II regions as seen by Herschel
P Tremblin, N Schneider, V Minier, P Didelon… - Astronomy & …, 2014 - aanda.org
Aims. Ionization feedback should impact the probability distribution function (PDF) of the
column density of cold dust around the ionized gas. We aim to quantify this effect and …
column density of cold dust around the ionized gas. We aim to quantify this effect and …