activity
20052016
most citedHi-GAL: the Herschel infrared Galactic Plane Survey

614 citations · 824 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2016★ 8 cited

The time evolution of HH 1 from four epochs of HST images

A. C. Raga, B. Reipurth, A. Esquivel +1

We present an analysis of four epochs of H and [S II] 6716/6731 HST images of HH 1. For determining proper motions we explore a new method based on analysis of spatially de…

astro-ph.GA2010★ 95 cited

Mapping the column density and dust temperature structure of IRDCs with Herschel

N. Peretto, G. A. Fuller, R. Plume +22

Infrared dark clouds (IRDCs) are cold and dense reservoirs of gas potentially available to form stars. Many of these clouds are likely to be pristine structures representing the in…

astro-ph.GA2010★ 614 cited

Hi-GAL: the Herschel infrared Galactic Plane Survey

S. Molinari, the Hi-GAL Consortium

Hi-GAL, the Herschel infrared Galactic Plane Survey, is an Open Time Key Project of the Herschel Space Observatory. It will make an unbiased photometric survey of the inner Galacti…

astro-ph2007★ 35 cited

Spitzer Observations of the HII Region NGC 2467: An Analysis of Triggered Star Formation

Keely D. Snider, J. Jeff Hester, Steven J. Desch +2

We present new Spitzer Space Telescope observations of the region NGC 2467, and use these observations to determine how the environment of an HII region affects the process of star…

astro-ph2006★ 21 cited

Silicate Emission Profiles from Low-Mass Protostellar Disks in the Orion Nebula: Evidence for Growth and Thermal Processing of Grains

R. Y. Shuping, Marc Kassis, Mark Morris +2

We present 8--13 micron low resolution spectra (R~100) of 8 low-mass protostellar objects ("proplyds") in the Orion Nebula using the Long Wavelength Spectrometer (LWS) at the W. M.…

astro-ph2005★ 51 cited

Multi-Generational Star Formation in L1551

Gerald H. Moriarty-Schieven, Doug Johnstone, John Bally +1

The L1551 molecular cloud contains two small clusters of Class 0 and I protostars, as well as a halo of more evolved Class II and III YSOs, indicating a current and at least one pa…