Publ. Astron. Soc. Pacific 107
December 1995
- 1995PASP..107.1131N
- The 75th Anniversary Astronomical Debate on the Distance Scale to Gamma-Ray Bursts: An Introduction
- ROBERT J. NEMIROFF
- 1995PASP..107.1133T
- The 1920 Shapley-Curtis Discussion: Background, Issues, and Aftermath
- VIRGINIA TRIMBLE
- 1995PASP..107.1145F
- Gamma-Ray Bursts: An Overview
- GERALD J. FISHMAN
- 1995PASP..107.1152L
- The Distance Scale to Gamma-Ray Bursts
- D. Q. LAMB
- 1995PASP..107.1167P
- How Far Away Are Gamma-Ray Bursters?
- BOHDAN PACZYNSKI
- 1995PASP..107.1176R
- Concluding Remarks
- MARTIN J. REES
- 1995PASP..107.1177L
- Aluminum-Oxygen Abundance Anticorrelations and Deep-Mixing Scenarios for Globular-Cluster Giants
- G. E. LANGER and R. D. HOFFMAN
- 1995PASP..107.1183P
- Superhumps in Cataclysmic Binaries. VIII. V1159 Orionis
- JOSEPH PATTERSON, F. JABLONSKI, C. KOEN, D. O'DONOGHUE, and DAVID R. SKILLMAN
- 1995PASP..107.1201P
- On the Erosion of the Helium Layer in White-Dwarf Nova Progenitors
- DINA PRIALNIK and MARIO LIVIO
- 1995PASP..107.1207N
- Toward a Unified View of Black-Hole High-Energy States
- MICHAEL A. NOWAK
- 1995PASP..107.1215T
- Composition and Evolution Patterns in the Old Open Cluster Melotte 66: Photoelectric (U)BV(RI) Photometry of 71 Stars
- BRUCE A. TWAROG, BARBARA J. ANTHONY TWAROG, and TIMOTHY G. HAWARDEN
- 1995PASP..107.1226P
- The Ohio State Imaging Fabry-Perot Spectrometer (IFPS)
- RICHARD W. POGGE, BRUCE ATWOOD, PAUL L. BYARD, THOMAS P. O'BRIEN, BRADLEY M. PETERSON, N. J. LAME, and JACK A. BALDWIN
- 1995PASP..107.1234M
- An Infrared Camera for the Palomar Observatory 60-inch Telescope
- D. C. MURPHY, S. E. PERSSON, MICHAEL A. PAHRE, A. SIVARAMAKRISHNAN, and S. G. DJORGOVSKI
- 1995PASP..107.1243W
- The SKICAT System for Processing and Analyzing Digital Imaging Sky Surveys
- NICHOLAS WEIR, USAMA M. FAYYAD, S. G. DJORGOVSKI, and JOSEPH RODEN
- 1995PASP..107.1255C
- Removal of Cosmic-Ray Events in Spectroscopic CCD Data
- B. F. W. CROKE
- 1995PASP..107.1259P
- Compact Groups of Galaxies
- RACHEL PILDIS
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