activity
20102026
most citedDynamic star formation in the massive DR21 filament

363 citations · 1.2k across the 17 of their papers we have counts for

collaborators

23 papers

astro-ph.IM2026

The environments forming stellar and planetary systems

Michael Kuffmeier, Jaime E. Pineda, Peter Schilke +29

How does a star's birth environment set the mass, angular momentum and chemical complexity delivered to its planet-forming disk, and thereby whether it builds planets, brown dwarfs…

astro-ph.IM2026

Chemical Demographics of Star-forming Regions

Maria N. Drozdovskaya, Timea Csengeri, Maria Teresa Beltrán +35

Our understanding of complex organic chemistry during the formation of stars and planets is shaped by a handful of cherry-picked sources with bright molecular emission lines. This…

astro-ph.IM2026

Star Formation across the Galaxy

Alvaro Sanchez-Monge, Henrik Beuther, Maryvonne Gerin +41

Star formation is both a multi-scale and highly dynamic process. It is regulated by the combination of gravity, turbulence, feedback and magnetic fields, which connect more than si…

astro-ph.IM2026

Frontiers of chemical complexity in the interstellar medium: unveiling the cosmic origins of life

Víctor M. Rivilla, Miguel Sanz-Novo, Maite Beltrán +33

The interstellar medium (ISM) contains a rich molecular inventory that provides a unique window into the chemistry operating during star and planet formation and its connection to…

astro-ph.IM2026

From local chemistry to galactic evolution: unlocking the power of interstellar isotopes with ALMA2040

Laura Colzi, Hayley A. Bunn, Víctor M. Rivilla +29

Molecular isotopic ratios provide a unique window into the chemical evolution of the interstellar medium, linking stellar nucleosynthesis and Galactic chemical evolution to the phy…

astro-ph.IM2026

Unveiling star formation at sub-solar metallicity with ALMA2040

Francesco Fontani, Frédérique Motte, Maria T. Beltrán +9

A fundamental question in astrophysics is whether the processes governing star formation are universal or depend on the physical conditions of their local galactic environment. The…

astro-ph.GA2026★ 1 cited

One-dimensional and time-dependent modelling of complex organic molecules in protostars

Le Ngoc Tram, Serena Viti, Katarzyna M. Dutkowska +5

Complex organic molecules (COMs), the building blocks of life, have been extensively detected under various physical conditions, from quiescent clouds to star-forming regions. They…

astro-ph.GA2025

Mass Assembly and Chemical Complexity in the Milky Way

Pamela Klaassen, David Eden, Alessio Traficante +13

(Sub-)millimeter spectral lines can be used not only to understand the chemical complexity and enrichment history of an observed portion of our Galaxy, but with spectrally resolved…

astro-ph.IM2025★ 2 cited

Identification of molecular line emission using Convolutional Neural Networks

Nina Kessler, Timea Csengeri, David Cornu +2

Complex organic molecules (COMs) are observed to be abundant in various astrophysical environments, in particular toward star forming regions they are observed both toward protoste…

astro-ph.GA2024

Global and Local Infall in the ASHES Sample (GLASHES). I. Pilot Study in G337.541

Kaho Morii, Patricio Sanhueza, Timea Csengeri +4

Recent high-angular-resolution observations indicate the need for core growth to form high-mass stars. To understand the gas dynamics at the core scale in the very early evolutiona…

astro-ph.GA2020★ 33 cited

The role of Galactic HII regions in the formation of filaments. High-resolution submilimeter imaging of RCW 120 with ArTéMiS

A. Zavagno, Ph. André, F. Schuller +13

Massive stars and their associated ionized (HII) regions could play a key role in the formation and evolution of filaments that host star formation. However, the properties of fila…

astro-ph.SR2017★ 18 cited

Cold CO gas in the envelopes of FU Orionis-type young eruptive stars

Á. Kóspál, P. Ábrahám, T. Csengeri +3

FUors are young stellar objects experiencing large optical outbursts due to highly enhanced accretion from the circumstellar disk onto the star. FUors are often surrounded by massi…

astro-ph.SR2015★ 1 cited

Discovery of molecular gas around HD 131835 in an APEX molecular line survey of bright debris disks

A. Moór, Th. Henning, A. Juhász +11

Debris disks are considered to be gas-poor, but recent observations revealed molecular or atomic gas in several 10-40 Myr old systems. We used the APEX and IRAM 30m radiotelescopes…

astro-ph.GA2014★ 64 cited

SiO emission from low- and high-velocity shocks in Cygnus-X massive dense clumps

A. Duarte-Cabral, S. Bontemps, F. Motte +4

We used PdBI observations of SiO (2-1) to investigate the morphology and profile of the SiO emission within several massive dense clumps (MDCs) in Cygnus-X. We find that most molec…

astro-ph.GA2014★ 19 cited

Water emission from the high-mass star-forming region IRAS 17233-3606. High water abundances at high velocities

S. Leurini, A. Gusdorf, F. Wyrowski +7

We investigate the physical and chemical processes at work during the formation of a massive protostar based on the observation of water in an outflow from a very young object prev…

astro-ph.SR2013★ 50 cited

ALMA continuum observations of a 30 Myr old gaseous debris disk around HD 21997

A. Moór, A. Juhász, Á. Kóspál +10

Circumstellar disks around stars older than 10 Myr are expected to be gas-poor. There are, however, two examples of old (30-40 Myr) debris-like disks containing a detectable amount…

astro-ph.SR2013★ 140 cited

ALMA observations of the molecular gas in the debris disk of the 30 Myr old star HD 21997

Á. Kóspál, A. Moór, A. Juhász +9

The 30 Myr old A3-type star HD 21997 is one of the two known debris dust disks having a measurable amount of cold molecular gas. With the goal of understanding the physical state,…

astro-ph.SR2013★ 52 cited

A resolved debris disk around the candidate planet-hosting star HD95086

A. Moór, P. Ábrahám, Á. Kóspál +11

Recently, a new planet candidate was discovered on direct images around the young (10-17 Myr) A-type star HD95086. The strong infrared excess of the system indicates that, similarl…

astro-ph.GA2013★ 155 cited

ATLASGAL --- properties of compact HII regions and their natal clumps

J. S. Urquhart, M. A. Thompson, T. J. T. Moore +13

We present a complete sample of molecular clumps containing compact and ultra-compact (UC) HII regions between \ell=10\degr and 60\degr\ and $|b|<1\degr, identified by combining th…

astro-ph.IM2013★ 56 cited

Characterization of the MALT90 Survey and the Mopra Telescope at 90 GHz

Jonathan B. Foster, Jill M. Rathborne, Patricio Sanhueza +23

We characterize the Millimeter Astronomy Legacy Team 90 GHz (MALT90) Survey and the Mopra telescope at 90 GHz. We combine repeated position-switched observations of the source G300…

astro-ph.SR2011★ 81 cited

Molecular gas in young debris disks

A. Moór, P. Ábrahám, A. Juhász +7

Gas-rich primordial disks and tenuous gas-poor debris disks are usually considered as two distinct evolutionary phases of the circumstellar matter. Interestingly, the debris disk a…

astro-ph.GA2010★ 118 cited

Gas dynamics in Massive Dense Cores in Cygnus-X

T. Csengeri, S. Bontemps, N. Schneider +2

We study the kinematic properties of dense gas surrounding massive protostars recognized by Bontemps et a. (2010) in a sample of five Massive Dense Cores in Cygnus-X. We investigat…

astro-ph.GA2010★ 363 cited

Dynamic star formation in the massive DR21 filament

N. Schneider, T. Csengeri, S. Bontemps +5

The formation of massive stars is a highly complex process in which it is not clear whether the star-forming gas is in global gravitational collapse or in an equilibrium state, sup…