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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
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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