activity
20172019
most citedThe Young Star Cluster population of M51 with LEGUS: I. A comprehensive study of cluster formation and evolution

68 citations · 171 across the 5 of their papers we have counts for

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Showing astro-ph.GAShow all

6 papers · 1 filter

astro-ph.GA20193 cited

Spatial segregation of massive clusters in dwarf galaxies

Bruce G. Elmegreen, A. Adamo, M. Boquien +14

The relative average minimum projected separations of star clusters in the Legacy ExtraGalactic UV Survey (LEGUS) and in tidal dwarfs around the interacting galaxy NGC 5291 are det…

astro-ph.GA201963 cited

Star Cluster Catalogs for the LEGUS Dwarf Galaxies

D. O. Cook, J. C. Lee, A. Adamo +62

We present the star cluster catalogs for 17 dwarf and irregular galaxies in the Treasury Program "Legacy ExtraGalactic UV Survey" (LEGUS). Cluster identification and photomet…

astro-ph.GA2018

Search For Star Cluster Age Gradients Across Spiral Arms of Three LEGUS Disk Galaxies

F. Shabani, E. K. Grebel, A. Pasquali +20

One of the main theories for explaining the formation of spiral arms in galaxies is the stationary density wave theory. This theory predicts the existence of an age gradient across…

astro-ph.GA2018

Extinction Maps and Dust-to-Gas Ratios in Nearby Galaxies with LEGUS

L. Kahre, R. A. Walterbos, H. Kim +44

We present a study of the dust-to-gas ratios in five nearby galaxies NGC 628 (M74), NGC 6503, NGC 7793, UGC 5139 (Holmberg I), and UGC 4305 (Holmberg II). Using Hubble Space Telesc…

astro-ph.GA201768 cited

The Young Star Cluster population of M51 with LEGUS: I. A comprehensive study of cluster formation and evolution

M. Messa, A. Adamo, G. Östlin +34

Recently acquired WFC3 UV (F275W and F336W) imaging mosaics under the Legacy Extragalactic UV Survey (LEGUS) combined with archival ACS data of M51 are used to study the young star…

astro-ph.GA2017

Effective Radii of Young, Massive Star Clusters in Two LEGUS Galaxies

J. E. Ryon, J. S. Gallagher, L. J. Smith +15

We present a study of the effective (half-light) radii and other structural properties of a systematically selected sample of young, massive star clusters (YMCs, $5\times10^3…