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ASTRONOMY AND ASTROPHYSICS Supplement Series, Volume 131, September 1998

CONTENTS

Pole coordinates and shape of 30 asteroids
C. Blanco and D. Riccioli

Comprehensive tables for the interpretation and modeling of the light curves of eclipsing binaries
A. Claret

Polarimetry of southern peculiar early-type stars
R.V. Yudin and A. Evans

A catalogue of accurate wavelengths in the optical spectrum of the Sun
C. Allende Prieto and R.J. García López

A new sample of faint Gigahertz Peaked Spectrum radio sources
I.A.G. Snellen, R.T. Schilizzi, A.G. de Bruyn, G.K. Miley, R.B. Rengelink, H.J. Röttgering and M.N. Bremer

50 tex2html_wrap_inline540as resolution VLBI images of AGN's at tex2html_wrap_inline5423mm
F.T. Rantakyrö, L.B. Båå th, D.C. Backer, R.S. Booth, J.E. Carlstrom, D.T. Emerson, M. Grewing, H. Hirabayashi, M.W. Hodges, M. Inoue, H. Kobayashi, T.P. Krichbaum, A.J. Kus, J.M. Moran, M. Morimoto, S. Padin, R.L. Plambeck, R. Predmore, A.E.E. Rogers, C. Schalinski, A. Witzel, D. Woody, M.C.H. Wright and A. Zensus

High resolution spectroscopy of the galactic candidate LBV MWC 314
A.S. Miroshnichenko, Y. Frémat, L. Houziaux, Y. Andrillat, E.L. Chentsov and V.G. Klochkova

B[e] stars. VI. MWC 297 = IRAS 18250-0351
Y. Andrillat and C. Jaschek

Integrated spectral study of reddened globular clusters and candidates
E. Bica, J.J. Clariá, A.E. Piatti and C. Bonatto

Atomic and molecular data

Atomic data from the IRON Project. XXIX. Radiative rates for transitions within the n = 2 complex in ions of the boron isoelectronic sequence
M.E. Galavís, C. Mendoza and C.J. Zeippen

Relativistic calculations on E1 transitions in As-like ions
E. Charro and I. Martín

Instruments and observational techniques

Floating mirror horizon. Theory and design
J. Suran

Data processing

A strategy for fitting partially blended ridges in GONG solar p-mode spectra
R. Howe and M.J. Thompson

The S2 baseband processing system for phase-coherent pulsar applications
R. Wietfeldt, W. Van Straten, D. Del Rizzo, N. Bartel, W. Cannon and A. Novikov

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