activity
20102026
most citedYSOVAR: the first sensitive, wide-area, mid-IR photometric monitoring of the ONC

234 citations · 2k across the 64 of their papers we have counts for

collaborators
Showing 2021Show all

6 papers · 1 filter

astro-ph.EP2021

The search for gas in debris discs: ALMA detection of CO gas in HD 36546

Isabel Rebollido, Álvaro Ribas, Itziar de Gregorio-Monsalvo +9

Debris discs represent the last stages of planet formation and as such are expected to be depleted of primordial gas. Nonetheless, in the last few years the presence of cold gas ha…

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.SR2021★ 16 cited

HS observations in young stellar disks in Taurus

P. Rivière-Marichalar, A. Fuente, R. Le Gal +7

Context. Studying gas chemistry in protoplanetary disks is key to understanding the process of planet formation. Sulfur chemistry in particular is poorly understood in interstellar…

astro-ph.SR2021★ 5 cited

The A-shell star Phi Leo revisited: its photospheric and circumstellar spectra

C. Eiroa, B. Montesinos, I. Rebollido +7

Variable red- and blue-shifted absorption features observed in the Ca ii K line towards the A-type shell star Leo have been suggested by us in a previous work to be likely due…

astro-ph.EP2021★ 19 cited

Observational signatures of eccentric Jupiters inside gas cavities in protoplanetary discs

Clément Baruteau, Gaylor Wafflard-Fernandez, Romane Le Gal +4

Predicting how a young planet shapes the gas and dust emission of its parent disc is key to constraining the presence of unseen planets in protoplanetary disc observations. We inve…