activity
20062009
most citedSpitzer SAGE Infrared Photometry of Massive Stars in the Large Magellanic Cloud

221 citations · 507 across the 8 of their papers we have counts for

collaborators

6 papers

astro-ph.CO200929 cited

Structures of Local Galaxies Compared to High Redshift Star-forming Galaxies

Sara M. Petty, Duilia F. de Mello, John S. Gallagher +4

The rest-frame far-ultraviolet (FUV) morphologies of 8 nearby interacting and starburst galaxies (Arp 269, M 82, Mrk 8, NGC 520, NGC 1068, NGC 3079, NGC 3310, NGC 7673) are compare…

astro-ph.SR2009221 cited

Spitzer SAGE Infrared Photometry of Massive Stars in the Large Magellanic Cloud

A. Z. Bonanos, D. L. Massa, M. Sewilo +11

We present a catalog of 1750 massive stars in the Large Magellanic Cloud, with accurate spectral types compiled from the literature, and a photometric catalog for a subset of 1268…

astro-ph200728 cited

Cluster and nebular properties of the central star-forming region of NGC 1140

S. L. Moll, S. Mengel, R. de Grijs +2

We present new high spatial resolution HST/ACS imaging of NGC 1140 and high spectral resolution VLT/UVES spectroscopy of its central star-forming region. The central region contain…

astro-ph200745 cited

Gemini GMOS/IFU spectroscopy of NGC 1569 - II: Mapping the roots of the galactic outflow

M. S. Westmoquette, L. J. Smith, J. S. Gallagher +1

We present a set of four Gemini-North GMOS/IFU observations of the central disturbed regions of the dwarf irregular starburst galaxy NGC 1569, surrounding the well-known super star…

astro-ph2007

Progressive star formation in the young SMC cluster NGC 602

Lynn Redding Carlson, E. Sabbi, M. Sirianni +9

NGC 602 is a young stellar cluster located in a peripheral region of the Small Magellanic Cloud known as the wing. Far from the main body of the galaxy and abutting the Magellanic…

astro-ph2006111 cited

Past and present star formation in the SMC: NGC 346 and its neighborhood

E. Sabbi, M. Sirianni, A. Nota +8

In the quest of understanding how star formation occurs and propagates in the low metallicity environment of the Small Magellanic Cloud (SMC), we acquired deep F555W (~V), and F814…