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CONTENTS
ASTRONOMY AND ASTROPHYSICS Supplement Series, Vol. 121, February 1997

CONTENTS

1. Spectroscopy of the open cluster Blanco 1. II. Htex2html_wrap_inline546 emission as an indicator of relative age
P.M. Panagi and M.A. O'Dell

2. Pre-main sequence candidates in the very young open cluster NGC 6611
D. de Winter, C. Koulis, P.S. Thé, M.E. van den Ancker, M.R. Pérez, and E.A. Bibo

3. GPM1 - a catalog of absolute proper motions of stars with respect to galaxies
S.P. Rybka and A.I. Yatsenko

4. UBV photometry of galactic foreground and LMC member stars. II. Galactic foreground stars (supplement)
H.-G. Grothues, M.O. Oestreicher, J. Gochermann, C. Tappert, A. Zaum, H.R. Brugger, and Th. Schmidt-Kaler

5. Ammonia observations towards molecular and optical outflows
G. Anglada, I. Sepúlveda, and J.F. Gómez

6. The peculiar B[e] star HD 45677. II. Photometric behaviour and spectroscopic properties
D. de Winter and M.E. van den Ancker

7. HST photometry: Can UV colors probe the galaxy ages?
C. Chiosi, A. Vallenari, and A. Bressan

8. A radio continuum study of the Magellanic Clouds. V. Catalogues of radio sources in the Small Magellanic Cloud at 1.42, 2.45, 4.75, 4.85 and 8.55 GHz
M.D. Filipovic, P.A. Jones, G.L. White, R.F. Haynes, U. Klein, and R. Wielebinski

9. Nonlinear investigation of the pulsational properties of RR Lyrae variables
G. Bono, F. Caputo, V. Castellani, and M. Marconi

10. Line-profile variations due to adiabatic non-radial pulsations in rotating stars. I. Observable characteristics of spheroidal modes
C. Schrijvers, J.H. Telting, C. Aerts, E. Ruymaekers, and H.F. Henrichs

11. Long-term monitoring of active stars. VI. tex2html_wrap_inline550 observations collected in Sep.-Oct. 1990
G. Cutispoto and G. Leto

Instruments and observational techniques

12. Deriving object visibilities from interferograms obtained with a fiber stellar interferometer
V. Coudé du Foresto, S. Ridgway, and J.-M. Mariotti

13. Sub-degree CMB anisotropy from space. II. In-flight calibration
M. Bersanelli, P.F. Muciaccia, P. Natoli, N. Vittorio, and N. Mandolesi



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