activity
20072025
most citedLegacy ExtraGalactic UV Survey with The Hubble Space Telescope. Stellar cluster catalogues and first insights into cluster formation and evolution in NGC 628

163 citations · 1.7k across the 45 of their papers we have counts for

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Showing 2017Show all

7 papers · 1 filter

astro-ph.SR2017★ 65 cited

Characterizing TW Hydra

Kimberly R. Sokal, Casey P. Deen, Gregory N. Mace +5

At 60 pc, TW Hydra (TW Hya) is the closest example of a star with a gas-rich protoplanetary disk, though TW Hya may be relatively old (3-15 Myr). As such, TW Hya is especially appe…

astro-ph.SR2017★ 7 cited

Inner warm disk of ESO H 279A revealed by NA I and CO overtone emission lines

A-Ran Lyo, Jongsoo Kim, Jae-Joon Lee +20

We present analysis of near-infrared, high-resolution spectroscopy towards the Flat-spectrum YSO (Young Stellar Object) ESO H 279a (1.5 solar mass) in the Serpens star forming r…

astro-ph.GA2017★ 54 cited

Hierarchical Star Formation in Turbulent Media: Evidence from Young Star Clusters

K. Grasha, B. G. Elmegreen, D. Calzetti +16

We present an analysis of the positions and ages of young star clusters in eight local galaxies to investigate the connection between the age difference and separation of cluster p…

astro-ph.GA2017★ 163 cited

Legacy ExtraGalactic UV Survey with The Hubble Space Telescope. Stellar cluster catalogues and first insights into cluster formation and evolution in NGC 628

A. Adamo, J. E. Ryon, M. Messa +53

We report the large effort which is producing comprehensive high-level young star cluster (YSC) catalogues for a significant fraction of galaxies observed with the Legacy ExtraGala…

astro-ph.SR2017★ 12 cited

The Spectrum of SS 433 in the H and K Bands

E. L. Robinson, C. S. Froning, D. T. Jaffe +5

SS~433 is an X-ray binary and the source of sub-relativistic, precessing, baryonic jets. We present high-resolution spectrograms of SS 433 in the infrared H and K bands. The spectr…

astro-ph.GA2017★ 37 cited

H2, CO, and Dust Absorption through Cold Molecular Clouds

John H. Lacy, Christopher Sneden, Hwihyun Kim +1

The abundance of H2 in molecular clouds, relative to the commonly used tracer CO, has only been measured toward a few embedded stars, which may be surrounded by atypical gas. We pr…