AAS 195th Meeting, January 2000
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All findings are embargoed until the time of presentation at the meeting.


Session 104. Dust and Star Formation in Galaxies

Display, Saturday, January 15, 2000, 9:20am-4:00pm, Grand Hall

104.01 The Correlation Between Radio and H\alpha and Radio Emission in Star Forming Galaxies
V. Andersen, S. Chin, L. Duvall, J. Laska (ASMS)
104.02 The Emission Line Ratio of NII/SII and Luminosity in Spirals
J.H. Kim, S.S. McGaugh (Department of Astronomy, University of Maryland)
104.03 Multi-Epoch 20 cm Observations of Maffei 2, IC 342, NGC 6946, and NGC 2903
N. A. Reddy, P. T. P. Ho, Q. Zhang (Harvard-Smithsonian Center for Astrophysics)
104.04 An HST Study of Star Formation in the Nuclear Ring of NGC 1326
R. Buta, P. Treuthardt, D. A. Crocker, G. G. Byrd (U. Alabama)
104.05 Dust Structures as Revealed by HST Imaging of Overlapping Galaxies
W.C. Keel, R.E. White III (U. Alabama)
104.06 An ISO View of Secular Evolution in Galaxy Pairs?
D.L. Domingue, J.W. Sulentic (U. Alabama), C. Xu, J.M. Mazzarella (IPAC/Caltech)
104.07 The Hubble Heritage Image of the Interacting Galaxies IC 2163 and NGC 2207
B.G. Elmegreen (IBM), D.M. Elmegreen (Vassar), M. Kaufman (Ohio State), E. Brinks (U. Guanajuato MX), C. Struck (Iowa State), M. Thomasson (Onsala Obs.), M. Klaric (Columbia, SC), Z. Levay, H.E. Bond, C.A. Christian, J. English, L. Frattare, F. Hamilton, K. Noll (STScI)
104.08 HST Observations of Dust and Star-Forming Regions in the Ocular Galaxy IC 2163 and Its Spiral Companion NGC2207
D.M. Elmegreen (Vassar), M. Kaufman (Ohio State), B.G. Elmegreen (IBM), E. Brinks (U. Guanajuato MX), C. Struck (Iowa State), M. Thomasson (Onsala Obs.), M. Klaric (Columbia, SC)
104.09 NICMOS Imaging of the Most Luminous Infrared Galaxies
D.C. Hines, F.J. Low (Steward Observatory), A.S. Evans (SUNY at Stony Brook), R.I. Thompson (Steward Observatory), N.Z. Scoville (CalTech), M.J. Rieke (Steward Observatory)
104.10 Sub-mm and Far-IR Imaging of Low Surface Brightness Galaxies
T. E. Pickering, J. M. van der Hulst (Kapteyn Institute)


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