activity
20132022
most citedGas phase Elemental abundances in Molecular cloudS (GEMS) I. The prototypical dark cloud TMC 1

128 citations · 774 across the 21 of their papers we have counts for

collaborators

21 papers

astro-ph.GA2022★ 5 cited

First images of the molecular gas around a born-again star revealed by ALMA

Daniel Tafoya, Jesús A. Toalá, Ramlal Unnikrishnan +7

Born-again stars allow probing stellar evolution in human timescales and provide the most promising path for the formation of hydrogen-deficient post-asymptotic giant branch object…

astro-ph.GA2021★ 12 cited

Probing the kinematics and chemistry of the hot core Mon R 2 IRS 3 using ALMA observations

A. Fuente, S. P. Treviño-Morales, T. Alonso-Albi +3

We present high angular resolution 1.1mm continuum and spectroscopic ALMA observations of the well-known massive proto-cluster Mon R 2 IRS 3.The continuum image at 1.1mm shows two…

astro-ph.GA2021★ 27 cited

Evolutionary view through the starless cores in Taurus: deuteration in TMC 1-C and TMC 1-CP

D. Navarro-Almaida, A. Fuente, L. Majumdar +11

The chemical and physical evolution of starless and pre-stellar cores are of paramount importance to understanding the process of star formation. The Taurus Molecular Cloud cores T…

astro-ph.GA2021★ 53 cited

Gas phase Elemental abundances in Molecular cloudS (GEMS). IV. Observational results and statistical trends

M. Rodríguez-Baras, A. Fuente, P. Riviére-Marichalar +33

Gas phase Elemental abundances in Molecular CloudS (GEMS) is an IRAM 30m Large Program designed to estimate the S, C, N, and O depletions and gas ionization degree, X(e-), in a set…

astro-ph.SR2020★ 39 cited

AB Aur, a Rosetta stone for studies of planet formation (I): chemical study of a planet-forming disk

Pablo Rivière Marichalar, Asunción Fuente, Romane Le Gal +7

AB Aur is a Herbig Ae star that hosts a prototypical transition disk. The disk shows a plethora of features connected with planet formation mechanisms. Understanding the physical a…

astro-ph.SR2020★ 4 cited

Gas kinematics of key prebiotic molecules in GV Tau N revealed with an ALMA, PdBI, and Herschel synergy

A. Fuente, S. P. Treviño-Morales, R. Le Gal +4

A large effort has been made to detect warm gas in the planet formation zone of circumstellar discs using space and ground-based near infrared facilities. GV Tau N, the most obscur…

astro-ph.GA2020★ 82 cited

Gas phase Elemental abundances in Molecular cloudS (GEMS). II. On the quest for the sulphur reservoir in molecular clouds: the case

D. Navarro-Almaida, R. Le Gal, A. Fuente +30

Sulphur is one of the most abundant elements in the Universe. Surprisingly, sulphuretted molecules are not as abundant as expected in the interstellar medium, and the identity of t…

astro-ph.GA2019★ 118 cited

Dynamics of cluster-forming hub-filament systems: The case of the high-mass star-forming complex Monoceros R2

S. P. Trevino-Morales, A. Fuente, A. Sanchez-Monge +15

High-mass stars and star clusters commonly form within hub-filament systems. Monoceros R2, harbors one of the closest such systems, making it an excellent target for case studies.…

astro-ph.SR2019★ 10 cited

Gas accretion within the dust cavity in AB Aur

Pablo Rivière-Marichalar, Asuncioón Fuente, Clément Baruteau +5

AB Aur is a Herbig Ae star hosting a well-known transitional disk. Because of its proximity and low inclination angle, it is an excellent object to study planet formation. Our goal…

astro-ph.GA2018★ 128 cited

Gas phase Elemental abundances in Molecular cloudS (GEMS) I. The prototypical dark cloud TMC 1

A. Fuente, D. Navarro, P. Caselli +30

GEMS is an IRAM 30m Large Program whose aim is determining the elemental depletions and the ionization fraction in a set of prototypical star-forming regions. This paper presents t…

astro-ph.SR2018★ 4 cited

Re-visiting the case of R Mon: Is CO removed at R<20 au?

T. Alonso-Albi, P. Riviere-Marichalar, A. Fuente +4

To our knowledge, R Mon is the only B0 star in which a gaseous Keplerian disk has been detected. However, there is some controversy about the spectral type of R Mon. Some authors p…

astro-ph.GA2017★ 35 cited

Far-infrared observations of a massive cluster forming in the Monoceros R2 filament hub

T. S. M. Rayner, M. J. Griffin, N. Schneider +29

We present far-infrared observations of Monoceros R2 (a giant molecular cloud at approximately 830 pc distance, containing several sites of active star formation), as observed at 7…

astro-ph.SR2016★ 9 cited

(sub)Millimeter Emission Lines of Molecules in Born-again Stars

D. Tafoya, J. A. Toalá, W. H. T. Vlemmings +7

The detection and study of molecular gas in born-again stars would be of great importance to understand their composition and chemical evolution. In addition, the molecular emissio…

astro-ph.GA2016★ 24 cited

The first CO+ image: Probing the HI/H2 layer around the ultracompact HII region Mon R2

S. P. Trevino-Morales, A. Fuente, A. Sanchez-Monge +12

The CO+ reactive ion is thought to be a tracer of the boundary between a HII region and the hot molecular gas. In this study, we present the spatial distribution of the CO+ rotatio…

astro-ph.GA2016★ 15 cited

Origin of the Lyman excess in early-type stars

R. Cesaroni, Á. Sánchez-Monge, M. T. Beltrán +3

Ionized regions around early-type stars are believed to be well-known objects, but until recently, our knowledge of the relation between the free-free radio emission and the IR emi…

astro-ph.GA2015★ 12 cited

The chemical footprint of the star formation feedback in M 82 on scales of 100 pc

D. Ginard, A. Fuente, S. García-Burillo +7

We present interferometric observations of the CN 1-0 (113.491 GHz), N2H+ 1-0 (93.173 GHz), H(41)a (92.034 GHz), CH3CN (91.987 GHz), CS 3-2 (146.969 GHz), c-C3H2 3-2 (145.089 GHz),…

astro-ph.GA2014★ 29 cited

Tentative Detection of the Nitrosylium Ion in Space

J. Cernicharo, S. Bailleux, E. Alekseev +8

We report the tentative detection in space of the nitrosylium ion, NO. The observations were performed towards the cold dense core Barnard 1-b. The identification of the NO…

astro-ph.GA2014★ 38 cited

Deuteration around the ultracompact HII region Mon R2

S. P. Treviño-Morales, P. Pilleri, A. Fuente +13

The massive star-forming region Mon R2 hosts the closest ultra-compact HII region that can be spatially resolved with current single-dish telescopes. We used the IRAM-30m telescope…

astro-ph.GA2013★ 25 cited

Kinematics of the ionized-to-neutral interfaces in Monoceros R2

P. Pilleri, A. Fuente, M. Gerin +10

Context. Monoceros R2 (Mon R2), at a distance of 830 pc, is the only ultra-compact H ii region (UC H ii) where its associated photon-dominated region (PDR) can be resolved with the…

astro-ph.GA2013★ 62 cited

Interstellar detection of c-C3D2

S. Spezzano, S. Brünken, P. Schilke +7

We report the first interstellar detection of c-C3D2. The doubly deuterated cyclopropenylidene, a carbene, has been detected toward the starless cores TMC- 1C and L1544 using the I…

astro-ph.GA2013★ 43 cited

Spatial distribution of small hydrocarbons in the neighborhood of the Ultra Compact HII region Monoceros R2

P. Pilleri, S. Treviño-Morales, A. Fuente +14

We study the chemistry of small hydrocarbons in the photon-dominated regions (PDRs) associated with the ultra-compact HII region Mon R2. Our goal is to determine the variations of…