90 citations · 277 across the 15 of their papers we have counts for
15 papers
An Infrared Census of Star Formation in the Horsehead Nebula
Brendan P. Bowler, William H. Waller, S. Thomas Megeath +2
At ~ 400 pc, the Horsehead Nebula (B33) is the closest radiatively-sculpted pillar to the Sun, but the state and extent of star formation in this structure is not well understood.…
HST-WFPC2 Observations of the Star Clusters in the Giant HII Regions of M33
Myung Gyoon Lee, Hong Soo Park, Sang Chul Kim +4
We present a photometric study of the stars in ionizing star clusters embedded in several giant HII regions of M33 (CC93, IC 142, NGC 595, MA2, NGC 604 and NGC 588). Our photometry…
Ultraviolet Signposts of Resonant Dynamics in the Starburst-Ringed Sab Galaxy, M94 (NGC 4736)
William H. Waller, Michael N. Fanelli, William C. Keel +10
M94 (NGC 4736) is investigated using images from the Ultraviolet Imaging Telescope (FUV-band), Hubble Space Telescope (NUV-band), Kitt Peak 0.9-m telescope (H-alpha, R, and I bands…
Far Ultraviolet Imagery of the Edge-On Spiral Galaxy NGC 4631
Andrew M. Smith, Nicholas R. Collins, William H. Waller +10
Far ultraviolet FUV imagery of the edge-on, Sc/SBd galaxy, NGC 4631 reveals very strong FUV emission, resulting from active star formation, uniformly distributed along the galactic…
Comparing Galaxy Morphology at Ultraviolet and Optical Wavelengths
L. E. Kuchinski, W. L. Freedman, Barry F. Madore +11
We have undertaken an imaging survey of 34 nearby galaxies in far-ultraviolet (FUV, ~1500A) and optical (UBVRI) passbands to characterize galaxy morphology as a function of wavelen…
Emission-Line Properties of the LMC Bubble N70
Brooke P. Skelton, William H. Waller, Richard F. Gelderman +4
We present a spectrophotometric imaging study of the emission bubble N70 (DEM 301) in the Large Magellanic Cloud. N70 is approximately 100 pc in size with a nearly circular shell-l…