activity
19992018
most citedALMA observations of the young protostellar system Barnard 1b: signatures of an incipient hot corino in B1b-S

54 citations · 179 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2018★ 54 cited

ALMA observations of the young protostellar system Barnard 1b: signatures of an incipient hot corino in B1b-S

N. Marcelino, M. Gerin, J. Cernicharo +8

The Barnard 1b core shows signatures of being at the earliest stages of low-mass star formation, with two extremely young and deeply embedded protostellar objects. Hence, this core…

astro-ph.SR2017★ 30 cited

Evidence for disks at an early stage in class 0 protostars?

M. Gerin, J. Pety, B. Commercon +8

The formation epoch of protostellar disks is debated because of the competing roles of rotation, turbulence, and magnetic fields in the early stages of low-mass star formation. Mag…

astro-ph.GA2017★ 13 cited

Chemical segregation in the young protostars Barnard 1b-N and S: evidence of pseudo-disk rotation in Barnard 1b-S

Asunción Fuente, Maryvonne Gerin, Jerome Pety +7

The extremely young Class 0 object B1b-S and the first hydrostatic core (FSHC) candidate, B1b-N, provide a unique opportunity to study the chemical changes produced in the elusive…

astro-ph.GA2016★ 18 cited

Star Formation and Feedback: A Molecular Outflow-Prestellar Core Interaction in L1689N

D. C. Lis, H. A. Wootten, M. Gerin +5

We present Herschel, ALMA Compact Array (ACA), and Caltech Submillimeter Observatory (CSO) observations of the prestellar core in L1689N, which has been suggested to be interacting…

astro-ph.GA2011★ 30 cited

High-resolution EVLA image of dimethyl ether (CH)O in Orion--KL

C. Favre, H. A. Wootten, A. J. Remijan +4

We report the first sub-arc second (0.65$\arcsec$ 0.51$\arcsec$) image of the dimethyl ether molecule, (CH)O, toward the Orion Kleinmann-Low nebula (Orion--KL)…

astro-ph1999★ 34 cited

VLA Observations of H2O Masers in the Class 0 Protostar S106 FIR: Evidence for a 10 AU-Scale Accelerating Jet-like Flow

R. S. Furuya, Y. Kitamura, M. Saito +2

We conducted VLA observations at 0".06 resolution of the 22 GHz water masers toward the Class 0 source S106 FIR (d=600 pc; 15" west of S106-IRS4) on two epochs separated by ~3 mont…