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20002026
most citedGLIMPSE: I. A SIRTF Legacy Project to Map the Inner Galaxy

1.4k citations · 14.3k across the 196 of their papers we have counts for

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Showing 2016Show all

6 papers · 1 filter

astro-ph.GA2016★ 57 cited

The Massive Protostellar Cluster NGC6334I at 220 AU Resolution: Discovery of Further Multiplicity, Diversity and a Hot Multi-Core

C. L. Brogan, T. R. Hunter, C. J. Cyganowski +3

We present VLA and ALMA imaging of the deeply-embedded protostellar cluster NGC6334I from 5 cm to 1.3 mm at angular resolutions as fine as 0.17 (220 AU). The dominant hot core MM1…

astro-ph.GA2016★ 27 cited

Studying Relation Between Star Formation and Molecular Clumps on Subparsec Scales in 30 Doradus

Omnarayani Nayak, Margaret Meixner, Remy Indebetouw +4

We present and molecular gas data observed by ALMA, massive early stage young stellar objects identified by applying color-magnitude cuts to \…

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★ 18 cited

The Prevalence and Impact of Wolf-Rayet Stars in Emerging Massive Star Clusters

Kimberly R. Sokal, Kelsey E. Johnson, Remy Indebetouw +1

We investigate Wolf-Rayet (WR) stars as a source of feedback contributing to the removal of natal material in the early evolution of massive star clusters. Despite previous work su…

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.GA2016★ 56 cited

A milestone toward understanding PDR properties in the extreme environment of LMC-30Dor

M. Chevance, S. C. Madden, V. Lebouteiller +11

More complete knowledge of galaxy evolution requires understanding the process of star formation and interaction between the interstellar radiation field and the interstellar mediu…