activity
20042018
most citedFirst Results from High Angular Resolution ALMA Observations Toward the HL Tau Region

1.2k citations · 2.2k across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.SR2018★ 16 cited

Sub-millimeter non-contaminated detection of the disk around TWA\,7 by ALMA

A. Bayo, J. Olofsson, L. Matra +9

Debris disks can be seen as the left-overs of giant planet formation and the possible nurseries of rocky planets. While M-type stars out-number more massive stars we know very litt…

astro-ph.SR2015★ 106 cited

Episodic molecular outflow in the very young protostellar cluster Serpens South

Adele L. Plunkett, Hector G. Arce, Diego Mardones +5

The loss of mass from protostars, in the form of a jet or outflow, is a necessary counterpart to protostellar mass accretion. Outflow ejection events probably vary in their velocit…

astro-ph.EP2015★ 20 cited

ALMA Observations of Asteroid 3 Juno at 60 Kilometer Resolution

ALMA Partnership, T. R. Hunter, R. Kneissl +67

We present Atacama Large Millimeter/submillimeter Array (ALMA) 1.3 mm continuum images of the asteroid 3 Juno obtained with an angular resolution of 0.042 arcseconds (60 km at 1.97…

astro-ph.SR2015★ 1.2k cited

First Results from High Angular Resolution ALMA Observations Toward the HL Tau Region

ALMA Partnership, C. L. Brogan, L. M. Perez +82

We present Atacama Large Millimeter/submillimeter Array (ALMA) observations from the 2014 Long Baseline Campaign in dust continuum and spectral line emission from the HL Tau region…

astro-ph.SR2011★ 18 cited

Benchmark cool companions: Ages and abundances for the PZ Tel system

James S. Jenkins, Yakiv V. Pavlenko, Oleksiy Ivanyuk +7

We present new ages and abundance measurements for the pre-main sequence star PZ Tel. PZ Tel was recently found to host a young and low-mass companion. Using FEROS spectra we have…

astro-ph.SR2010★ 166 cited

The effect of magnetic activity on low-mass stars in eclipsing binaries

J. C. Morales, J. Gallardo, I. Ribas +3

In recent years, analyses of eclipsing binary systems have unveiled differences between the observed fundamental properties of low-mass stars and those predicted by stellar structu…