activity
20092026
most citedThe identification of filaments on far infrared and submillimiter images. Morphology, physical conditions and relation with star formation of filamentary structure

144 citations · 2.6k across the 65 of their papers we have counts for

collaborators
Showing 2017Show all

5 papers · 1 filter

astro-ph.SR2017★ 24 cited

The circumestellar disk of the B0 protostar powering the HH 80-81 radio jet

J. M. Girart, R. Estalella, M. Fernández-López +6

We present subarcsecond angular resolution observations carried out with the Submillimeter Array (SMA) at 880 m centered at the B0-type protostar GGD27~MM1, the driving source o…

astro-ph.GA2017★ 16 cited

The L1157-B1 astrochemical laboratory: testing the origin of DCN

G. Busquet, F. Fontani, S. Viti +4

L1157-B1 is the brightest shocked region of the large-scale molecular outflow, considered the prototype of chemically rich outflows, being the ideal laboratory to study how shocks…

astro-ph.GA2017★ 49 cited

Thermal Jeans fragmentation within 1000 AU in OMC-1S

Aina Palau, Luis A. Zapata, Carlos G. Roman-Zuniga +6

We present subarcsecond 1.3 mm continuum ALMA observations towards the Orion Molecular Cloud 1 South (OMC-1S) region, down to a spatial resolution of 74 AU, which reveal a total of…

astro-ph.GA2017★ 47 cited

Cloud structure of three Galactic infrared dark star-forming regions from combining ground and space based bolometric observations

Yuxin Lin, Hauyu Baobab Liu, James E. Dale +12

We have modified the iterative procedure introduced by Lin et al. (2016), to systematically combine the submm images taken from ground based (e.g., CSO, JCMT, APEX) and space (e.g.…

astro-ph.GA2017★ 9 cited

The shocked gas of the BHR71 outflow observed by Herschel: indirect evidence for an atomic jet

M. Benedettini, A. Gusdorf, B. Nisini +7

In the BHR71 region, two low-mass protostars drive two distinguishable outflows. They constitute an ideal laboratory to investigate the effects of shock chemistry and the mechanism…