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20042026
most citedGravity or turbulence? -III. Evidence of pure thermal Jeans fragmentation at ~0.1 pc scale

116 citations · 3.5k across the 104 of their papers we have counts for

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Showing 2015Show all

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astro-ph.SR2015★ 53 cited

Two-level hierarchical fragmentation in the Orion Molecular Cloud 1 northern filament

P. S. Teixeira, S. Takahashi, L. A. Zapata +1

[Abridged] We have recently reported on the collapse and fragmentation properties of the northernmost part of this structure, located ~2.4pc north of Orion KL -- the Orion Molecula…

astro-ph.SR2015★ 22 cited

The Gould's Belt Very Large Array Survey V: The Perseus Region

Gerardo Pech, Laurent Loinard, Sergio A. Dzib +12

We present multi-epoch, large-scale ( 2000 arcmin), fairly deep ( 16 Jy), high-resolution ( 1") radio observations of the Perseus star-forming complex ob…

astro-ph.GA2015★ 16 cited

Complex molecules in W51 North region

Jialei Rong, Sheng-Li Qin, Luis A. Zapata +6

We present Submillimeter Array (SMA) molecular line observations in two 2 GHz-wide bands centered at 217.5 and 227.5 GHz, toward the massive star forming region W51 North. We ident…

astro-ph.SR2015★ 8 cited

Radio monitoring of the periodically variable IR source LRLL 54361: No direct correlation between the radio and IR emissions

Jan Forbrich, Luis F. Rodríguez, Aina Palau +3

LRLL 54361 is an infrared source located in the star forming region IC 348 SW. Remarkably, its infrared luminosity increases by a factor of 10 during roughly one week every 25.34 d…

astro-ph.SR2015★ 15 cited

Origin and kinematics of the eruptive flow from XZ Tau revealed by ALMA

Luis A. Zapata, Roberto Galvan-Madrid, Carlos Carrasco-Gonzalez +6

We present high angular resolution (0.94) CO(1-0) Atacama Large Millimeter/Submillimeter Array (ALMA) observations obtained during the 2014 long baseline campaign f…

astro-ph.GA2015

Pre- and Post-burst Radio Observations of the Class 0 Protostar HOPS 383 in Orion

Roberto Galván-Madrid, Luis F. Rodríguez, Hauyu B. Liu +5

There is increasing evidence that episodic accretion is a common phenomenon in Young Stellar Objects (YSOs). Recently, the source HOPS 383 in Orion was reported to have a $\times 3…