activity
19962026
most citedM32+/-1

217 citations · 1.1k across the 46 of their papers we have counts for

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Showing astro-ph.COShow all

6 papers · 1 filter

astro-ph.CO2013★ 13 cited

Tidal Tails of Minor Mergers II: Comparing Star Formation in the Tidal Tails of NGC 2782

Karen Knierman, Paul Scowen, Todd Veach +5

The peculiar spiral NGC 2782 is the result of a minor merger with a mass ratio ~4:1 occurring ~200 Myr ago. This merger produced a molecular and HI rich, optically bright Eastern t…

astro-ph.CO2012★ 16 cited

Tidal Tails of Minor Mergers: Star Formation Efficiency in the Western Tail of NGC 2782

Karen Knierman, Patricia Knezek, Paul Scowen +2

While major mergers and their tidal debris are well studied, they are less common than minor mergers (mass ratios < 0.3). The peculiar spiral NGC 2782 is the result of a merger bet…

astro-ph.CO2010★ 20 cited

Mapping the Recent Star Formation History of the Disk of M51

Catherine C. Kaleida, Paul A. Scowen

Using data acquired as part of a unique Hubble Heritage imaging program of broadband colors of the interacting spiral system M51/NGC 5195, we have conducted a photometric study of…

astro-ph.CO2009★ 1 cited

Galaxy Assembly and SMBH/AGN-growth from Cosmic Dawn to the End of Reionization

Rolf A. Jansen, Rogier Windhorst, James Rhoads +5

[abridged] We propose a tiered, UV--near-IR, cosmological broad- and medium-band imaging and grism survey that covers ~10 deg^2 in two epochs to m_AB=28, ~3 deg^2 in seven epochs t…

astro-ph.CO2009

A Systematic Study of the Stellar Populations and ISM in Galaxies out to the Virgo Cluster

Rolf A. Jansen, Paul Scowen, Matthew Beasley +6

We present a compelling case for a systematic and comprehensive study of the resolved and unresolved stellar populations, ISM, and immediate environments of galaxies throughout the…

astro-ph.CO2009★ 1 cited

The Magellanic Clouds Survey: a Bridge to Nearby Galaxies

Paul A. Scowen, Rolf Jansen, Matthew Beasley +7

We outline to the community the value of a Magellanic Clouds Survey that consists of three components: I) a complete-area, high resolution, multi-band UV-near-IR broadband survey;…