activity
20152020
most citedThe Herschel Orion Protostar Survey: Spectral Energy Distributions and Fits Using a Grid of Protostellar Models

229 citations · 488 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2020★ 11 cited

An APEX survey of outflow and infall toward the youngest protostars in Orion

Z. Nagy, A. Menechella, S. T. Megeath +7

We aim to characterize the outflow properties of a sample of early Class 0 phase low-mass protostars in Orion first identified by the Herschel Space Observatory. We also look for s…

astro-ph.IM2020★ 54 cited

SciServer: a Science Platform for Astronomy and Beyond

Manuchehr Taghizadeh-Popp, Jai Won Kim, Gerard Lemson +8

We present SciServer, a science platform built and supported by the Institute for Data Intensive Engineering and Science at the Johns Hopkins University. SciServer builds upon and…

astro-ph.GA2017

HOPS 108: Star-formation triggered by a non-thermal jet?

A. K. Díaz Rodríguez, M. Osorio, G. Anglada +12

The nature of the far-IR source HOPS 108 has been a matter of debate in the last years. Previous radio observations detected a 3.6 cm source (VLA 12), coincident with HOPS 108, tha…

astro-ph.SR2017★ 95 cited

The Herschel Orion Protostar Survey: Luminosity and Envelope Evolution

William J. Fischer, S. Thomas Megeath, Elise Furlan +12

The Herschel Orion Protostar Survey obtained well-sampled 1.2 - 870 micron spectral energy distributions (SEDs) of over 300 protostars in the Orion molecular clouds, home to most o…

astro-ph.SR2016★ 229 cited

The Herschel Orion Protostar Survey: Spectral Energy Distributions and Fits Using a Grid of Protostellar Models

E. Furlan, W. J. Fischer, B. Ali +12

We present key results from the Herschel Orion Protostar Survey (HOPS): spectral energy distributions (SEDs) and model fits of 330 young stellar objects, predominantly protostars,…

astro-ph.SR2015★ 99 cited

HOPS 383: An Outbursting Class 0 Protostar in Orion

Emily J. Safron, William J. Fischer, S. Thomas Megeath +11

We report the dramatic mid-infrared brightening between 2004 and 2006 of HOPS 383, a deeply embedded protostar adjacent to NGC 1977 in Orion. By 2008, the source became a factor of…