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ASTRONOMY AND ASTROPHYSICS Supplement Series, Volume 135, March I 1999

CONTENTS

JHK photometry of symbiotic stars
U.S. Kamath and N.M. Ashok

Planetary nebulae in M 32 and the bulge of M 31: Line intensities and oxygen abundances
M.G. Richer, G. Stasinska and M.L. McCall

A list of nearby dwarf galaxies towards the Local Void in Hercules-Aquila
V.E. Karachentseva, I.D. Karachentsev and G.M. Richter

Solar diameter observations at Observatório Nacional in 1997-1998
E.G. Jilinski, S. Puliaev, J.L. Penna, A.H. Andrei and F. Laclare

Mining in the Hipparcos raw data
J.L. Falin and F. Mignard

High X-ray-to-optical flux ratio RASS-BSC sources. I. The optical identification
L. Cao, J.-Y. Wei and J.-Y. Hu

Nançay ``blind'' 21 cm line survey of the Canes Venatici group region
R.C. Kraan-Korteweg, W. van Driel, F. Briggs, B. Binggeli and T.I. Mostefaoui

Gigahertz peaked spectrum sources from the Jodrell Bank-VLA astrometric survey. I. Sources in the region tex2html_wrap_inline560
A. Marecki, H. Falcke, J. Niezgoda, S.T. Garrington and A.R. Patnaik

Alpha Cygnids - a possible July minor meteor shower
A. Olech, M. Gajos and M. Jurek

Infrared imaging of WENSS radio sources
D. Villani and S. di Serego Alighieri

The ROSAT all-sky survey catalogue of the nearby stars
M. Hünsch, J.H.M.M. Schmitt, M.F. Sterzik and W. Voges

Atomic and molecular data

CHIANTI - an atomic database for emission lines. III. Continuum radiation and extension of the ion database
E. Landi, M. Landini, K.P. Dere, P.R. Young and H.E. Mason

Atomic data from the Iron Project. XXXV. Relativistic fine structure oscillator strengths for Fe XXIV and Fe XXV
S.N. Nahar and A.K. Pradhan

Recombination line intensities for hydrogenic ions: The fine-structure components of HI and HeII
R.E.S. Clegg, S. Miller, P.J. Storey and R. Kisielius

Instruments and observational techniques

Pile-up on X-ray CCD instruments
J. Ballet

Computational methods

An improved method for the determination of the orbital parameters of a binary system that contains a pulsating component
G. Molenberghs, C. Aerts and P. De Cat

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Copyright by the European Southern Observatory (ESO)