activity
20072014
most citedThe Nature of Transition Circumstellar Disks I. The Ophiuchus Molecular Cloud

156 citations · 473 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.GA2014★ 4 cited

Molecular gas associated with IRAS 10361-5830

M. M. Vazzano, C. E. Cappa, J. Vasquez +3

We analyze the distribution of the molecular gas and the dust in the molecular clump linked to IRAS 10361-5830, located in the environs of the bubble-shaped HII region Gum 31 in th…

astro-ph.GA2014★ 3 cited

Molecules, dust, and protostars in NGC 3503

N. U. Duronea, J. Vasquez, G. A. Romero +3

We are presenting here a follow-up study of the molecular gas and dust in the environs of the star forming region NGC 3503. This study aims at dealing with the interaction of NGC 3…

astro-ph.GA2013★ 3 cited

Star forming regions linked to RCW78 and the discovery of a new IR bubble

C. E. Cappa, M. Rubio, G. A. Romero +2

With the aim of investigating the presence of molecular and dust clumps linked to two star forming regions identified in the expanding molecular envelope of the stellar wind bubble…

astro-ph.EP2012★ 30 cited

Submillimeter Array Observations of the RX J1633.9-2442 Transition Disk: Evidence for Multiple Planets in the Making

Lucas A. Cieza, Geoffrey S. Mathews, Jonathan P. Williams +6

We present continuum high resolution Submillimeter Array (SMA) observations of the transition disk object RX J1633.9-2442, which is located in the Ophiuchus molecular cloud and has…

astro-ph.SR2012★ 91 cited

The Nature of Transition Circumstellar Disks III. Perseus, Taurus, and Auriga

Lucas A. Cieza, Matthias R. Schreiber, Gisela A. Romero +3

As part of an ongoing program aiming to characterize a large number of Spitzer-selected transition disks (disks with reduced levels of near-IR and/or mid- IR excess emission), we h…

astro-ph.SR2012★ 76 cited

The Nature of Transition Circumstellar Disks II. Southern Molecular Clouds

Gisela A. Romero, Matthias R. Schreiber, Lucas A. Cieza +5

Transition disk objects are pre-main-sequence stars with little or no near-IR excess and significant far-IR excess, implying inner opacity holes in their disks. Here we present a m…