activity
19952023
most citedSpitzer Survey of the Large Magellanic Cloud, Surveying the Agents of a Galaxy's Evolution (SAGE) I: Overview and Initial Results

718 citations · 7.3k across the 122 of their papers we have counts for

collaborators
Showing 2016Show all

5 papers · 1 filter

astro-ph.GA2016★ 14 cited

The location, clustering, and propagation of massive star formation in giant molecular clouds

B. B. Ochsendorf, M. Meixner, J. Chastenet +2

Massive stars are key players in the evolution of galaxies, yet their formation pathway remains unclear. In this work, we use data from several galaxy-wide surveys to build an unbi…

astro-ph.SR2016★ 18 cited

The mass-loss rates of red supergiants at low metallicity: Detection of rotational CO emission from two red supergiants in the Large Magellanic Cloud

Mikako Matsuura, B. Sargent, Bruce Swinyard +9

Using the PACS and SPIRE spectrometers on-board the Herschel Space Observatory, we obtained spectra of two red supergiants (RSGs) in the Large Magellanic Cloud (LMC). Multiple rota…

astro-ph.GA2016★ 22 cited

Radiative and mechanical feedback into the molecular gas in the Large Magellanic Cloud. I. N159W

Min-Young Lee, Suzanne Madden, Vianney Lebouteiller +25

We present Herschel SPIRE Fourier Transform Spectrometer (FTS) observations of N159W, an active star-forming region in the Large Magellanic Cloud (LMC). In our observations, a numb…

astro-ph.GA2016★ 51 cited

Kinematic Structure of Molecular Gas around High-mass Star YSO, Papillon Nebula, in N159 East in the Large Magellanic Cloud

Kazuya Saigo, Toshikazu Onishi, Omnarayani Nayak +20

We present the ALMA Band 3 and Band 6 results of 12CO(2-1), 13$CO(2-1), H30alpha recombination line, free-free emission around 98 GHz, and the dust thermal emission around 230 GHz…

astro-ph.SR2016★ 77 cited

The evolved-star dust budget of the Small Magellanic Cloud: the critical role of a few key players

Sundar Srinivasan, Martha L. Boyer, Francisca Kemper +3

The lifecycle of dust in the interstellar medium (ISM) is heavily influenced by outflows from asymptotic giant branch (AGB) and red supergiant (RSG) stars, a large fraction of whic…