activity
20102026
most citedEvolution of PAHs in photodissociation regions: Hydrogenation and charge states

183 citations · 1.5k across the 43 of their papers we have counts for

collaborators

43 papers

astro-ph.GA2026

Statistical analysis of the relative orientations between filaments and magnetic fields using Herschel and Planck data in star-forming regions

Jonathan Oers, Isabelle Ristorcelli, Katia Ferrière +4

Observations and simulations of the interstellar medium both suggest that magnetic fields play a key role in the formation and evolution of filaments and in the process of star for…

astro-ph.GA2026

B-Fields and Star Formation across Scales with TRAO (B-FROST): CO Abundances, Dynamics and Relative Orientations in the Translucent High Latitude Cloud MBM12

J. M. Vorster, J. Montillaud, M. Juvela +14

In our Galaxy, the average star formation efficiency is of the order of a few percent. We investigated the high-latitude molecular cloud MBM12 as part of the B-fields and star form…

astro-ph.GA2024

The magnetic field in quiescent star-forming filament G16.96+0.27

Qi-Lao Gu, Tie Liu, Zhi-Qiang Shen +20

We present 850 μm thermal dust polarization observations with a resolution of 14.4"(~ 0.13 pc) towards an infrared dark cloud G16.96+0.27 using JCMT/POL-2. The average magnetic fie…

astro-ph.GA2024

The magnetic field in colliding filaments G202.3+2.5

Qi-Lao Gu, Tie Liu, Pak Shing Li +19

We observe the magnetic field morphology towards a nearby star-forming filamentary cloud, G202.3+2.5, by the JCMT/POL-2 850 μm thermal dust polarization observation with an angular…

astro-ph.GA2022★ 34 cited

A self-consistent dynamical model of the Milky Way disc adjusted to Gaia data

A. C. Robin, O. Bienaymé, J. B. Salomon +6

This paper shows how a self-consistent dynamical model can be obtained by fitting the gravitational potential of the Milky Way to the stellar kinematics and densities from Gaia dat…

astro-ph.GA2022★ 7 cited

Chemical exploration of Galactic cold cores

Chenlin Zhou, Charlotte Vastel, Julien Montillaud +6

A solar-type system starts from an initial molecular core that acquires organic complexity as it evolves. The so-called prestellar cores that can be studied are rare, which has ham…

astro-ph.GA2022★ 1 cited

3D extinction mapping of the Milky Way using Convolutional Neural Networks: Presentation of the method and demonstration in the Carina Arm region

D. Cornu, J. Montillaud, D. J. Marshall +2

Context. Several methods have been proposed to build 3D extinction maps of the Milky Way (MW), most often based on Bayesian approaches. Although some studies employed machine learn…

astro-ph.GA2021★ 31 cited

Deciphering the evolution of the Milky Way discs: Gaia APOGEE Kepler giant stars and the Besançon Galaxy Model

N. Lagarde, C. Reylé, C. Chiappini +13

We investigate the properties of the double sequences of the Milky Way discs visible in the [/Fe] vs [Fe/H] diagram. In the framework of Galactic formation and evolution, we dis…

astro-ph.GA2021★ 9 cited

Characterization of dense Planck clumps observed with Herschel and SCUBA-2

E. Mannfors, M. Juvela, L. Bronfman +15

We aim to characterize a diverse selection of dense, potentially star-forming cores, clumps, and clouds within the Milky Way in terms of their dust emission and SF activity. We stu…

astro-ph.GA2020★ 27 cited

ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): Detection of extremely high density compact structure of prestellar cores and multiple substructures within

Dipen Sahu, Sheng-Yuan Liu, Tie Liu +38

Prestellar cores are self-gravitating dense and cold structures within molecular clouds where future stars are born. They are expected, at the stage of transitioning to the protost…

astro-ph.GA2020★ 17 cited

A neural network-based methodology to select young stellar object candidates from IR surveys

David Cornu, Julien Montillaud

Observed Young Stellar Objects (YSOs) are used to study star formation and characterize star forming regions. For this purpose, YSO candidate catalogs are compiled from various sur…

astro-ph.IM2020

Space Project for Astrophysical and Cosmological Exploration (SPACE), an ESA stand-alone mission and a possible contribution to the Origins Space Telescope

Denis Burgarella, Andrew Bunker, Rychard Bouwens +30

We propose a new mission called Space Project for Astrophysical and Cosmological Exploration (SPACE) as part on the ESA long term planning Voyage 2050 programme. SPACE will study g…

astro-ph.GA2020★ 17 cited

Large-scale magnetic field in the Monoceros OB-1 East molecular cloud

D. Alina, J. Montillaud, Y. Hu +7

We study the large-scale magnetic field structure and its interplay with the gas dynamics in the Monoceros OB1 East molecular cloud. We combine observations of dust polarised emiss…

astro-ph.GA2019★ 33 cited

Multi-scale analysis of the Monoceros OB 1 star-forming region: II. Colliding filaments in the Monoceros OB1 molecular cloud

Julien Montillaud, Mika Juvela, Charlotte Vastel +24

We started a multi-scale analysis of G202.3+2.5, an intertwined filamentary region of Monoceros OB1. In Paper I, we examined the distributions of dense cores and protostars and fou…

astro-ph.GA2019★ 16 cited

Multi-scale analysis of the Monoceros OB 1 star-forming region: I. The dense core population

Julien Montillaud, Mika Juvela, Charlotte Vastel +24

Current theories and models attempt to explain star formation globally, from core scales to giant molecular cloud scales. A multi-scale observational characterisation of an entire…

astro-ph.GA2019★ 53 cited

Magnetic fields in the infrared dark cloud G34.43+0.24

Archana Soam, Tie Liu, B-G Andersson +11

We present the B-fields mapped in IRDC G34.43+0.24 using 850\,m polarized dust emission observed with the POL-2 instrument at JCMT. We examine the magnetic field geometries and…

astro-ph.GA2019

Galactic continuum surveys with the new 850 micron MKID camera at the EAO/JCMT 15-m telescope

Tie Liu, Di Li, David Eden +24

This white paper gives a brief summary of Galactic continuum surveys with the next generation 850 micron camera at the James Clerk Maxwell Telescope (JCMT) in the next decade. This…

astro-ph.GA2019★ 3 cited

Submillimeter continuum variability in Planck Galactic cold clumps

Geumsook Park, Kee-Tae Kim, Doug Johnstone +20

In the early stages of star formation, a protostar is deeply embedded in an optically thick envelope such that it is not directly observable. Variations in the protostellar accreti…

astro-ph.GA2019★ 39 cited

SCOPE: SCUBA-2 Continuum Observations of Pre-protostellar Evolution - Survey Description and Compact Source Catalogue

D. J. Eden, Tie Liu, Kee-Tae Kim +157

We present the first release of the data and compact-source catalogue for the JCMT Large Program SCUBA-2 Continuum Observations of Pre-protostellar Evolution (SCOPE). SCOPE consist…

astro-ph.GA2018★ 33 cited

Dust spectrum and polarisation at 850 um in the massive IRDC G035.39-00.33

Mika Juvela, Vincent Guillet, Tie Liu +18

The dust sub-millimetre polarisation of star-forming clouds carries information on dust and the role of magnetic fields in cloud evolution. With observations of a dense filamentary…

astro-ph.GA2018★ 28 cited

The properties of Planck Galactic cold clumps in the L1495 dark cloud

Mengyao Tang, Tie Liu, Sheng-Li Qin +19

Planck Galactic Cold Clumps (PGCCs) possibly represent the early stages of star formation. To understand better the properties of PGCCs, we studied 16 PGCCs in the L1495 cloud with…

astro-ph.GA2018★ 21 cited

Galactic cold cores IX. Column density structures and radiative transfer modelling

M. Juvela, J. Malinen, J. Montillaud +3

The Galactic Cold Cores (GCC) project has made Herschel observations of interstellar clouds where Planck detected compact sources of cold dust emission. Our aim is to characterise…

astro-ph.GA2018★ 104 cited

Structure of photodissociation fronts in star-forming regions revealed by observations of high-J CO emission lines with Herschel

C. Joblin, E. Bron, C. Pinto +17

In bright photodissociation regions (PDRs) associated to massive star formation, the presence of dense "clumps" that are immersed in a less dense interclump medium is often propose…

astro-ph.GA2017★ 10 cited

A CO survey on a sample of Herschel cold clumps

O. Fehér, M. Juvela, T. Lunttila +4

The physical state of cold cloud clumps has a great impact on the process and efficiency of star formation and the masses of the forming stars inside these objects. The sub-millime…