A Magyar Tudományos Akadémia Csillagvizsgáló Intézetének Közleményei, 15 (1) - 2026. pp. 1-236. ISSN 238-2091
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Abstract
No. 106. Unpublished observations of pulsating stars by Margit Paparó TABLE OF CONTENTS ABSTRACT INTRODUCTION DATA OF δ Scuti STARS θ 2 Tau = 78 Tau (1980-1986) FM Com (1982-1989) 57 Tau (1981-1995) VW Ari (1982-1994) θ Tuc (1993) CoRoT 10274568, alias Konkoly21 (2011-2012) SHORTER RUNS ON δ Scuti STARS DL Dra = HR 5492 or ER Dra = HR 5437 (1986-1988) KW 385 = HD 73890 (1990) Praesepe stars: KW 445, KW 323, KW 207 (1985-1991) 4 CVn and HD 108100 (1996) ǫ Cep (1981-1988) DATA OF OTHER TYPE OF STARS 25 Cyg (1992) (Be star) 29 Cyg (1996) (λ Boo-type) ν and μ Eri (2002-2003) (β Cep and SPB) ψ and ζ Tau (1991) (Be-type) TV Boo (1992) (RRc type) AC And (1992) (RR Lyrae) GD 154 (2006) (white dwarf) DK Cygni (1985) (W UMa type) 8 Draconis (2003) (γ Doradus type) ACKNOWLEDGEMENTS REFERENCES Abstract Unpublished photoelectric data of pulsating variable stars obtained in Hungary between 1980 and 2014 are presented here. Besides the data of the mainly investigated δ Scuti stars, many other types of pulsating stars are included (Be, λ Boo, β Cep, RR Lyr, WD, γ Dor and W UMa). Observations obtained in the frame of international cooperations, both with Hungarian or foreign leadership, are also shown. The long timebase is essential for variable star research besides the continuous but short timespan measurements of space missions (MOST, CoRoT, Kepler, TESS). The main aim of this publication is to preserve the unpublished old data. Some of our collaborators did not publish the data, some lost it in computer crash. Due to our proper preservation over consecutive technical recordings, we included their data (with permission) in this publication. Johnson UBVRI colours were used in Hungary, however, Strömgren ubvy colours with b-y, m 1 and c 1 indices are given in the case of non-Hungarian contributions. The online paper contains the light curves not only for the variable stars but the comparisons and check stars, showing the quality of observations. Besides the table of this online paper, the data will also be uploaded to the VizieR archive in a machine-readable format.
| Item Type: | Journal |
|---|---|
| Publisher: | Konkoly Observatory, MTA |
| Additional Information: | Communications from the Konkoly Observatory / Mitteilungen der Konkoly Sternwarte |
| Subjects: | Q Science / természettudomány > QB Astronomy, Astrophysics / csillagászat, asztrofizika |
| Depositing User: | Andras Holl |
| Date Deposited: | 15 Sep 2026 11:15 |
| Last Modified: | 15 Sep 2026 18:15 |
| URI: | https://real-j.mtak.hu/id/eprint/30694 |
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