Search catalogue
J/A+AS/132/93 Hipparcos photometry of CP stars (Adelman 1998)
On the Hipparcos photometry of Chemically Peculiar B, A, and F stars Adelman S.J. <Astron. Astrophys. Suppl. Ser. 132, 93 (1998)> =1998A&AS..132...93A (SIMBAD/NED BibCode)
ADC_Keywords: Stars, peculiar ; Stars, early-type ; Photometry Keywords: stars: early-type - stars: chemically peculiar Abstract: The Hipparcos photometry of the chemically peculiar main-sequence B, A and F stars are examined for variability. Some non-magnetic CP stars, Mercury-Manganese and metallic-line stars, which according to canonical wisdom should not be variable, may be variable and are identified for further study. Some potentially important magnetic CP stars are noted. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 52 120 Hipparcos HgMn star photometry table2.dat 42 192 Hipparcos Am star photometry table3.dat 42 331 Hipparcos magnetic CP star photometry
See also: I/239 : The Hipparcos and Tycho Catalogues (ESA 1997) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 9 A9 --- HR/HD HR (Cat. V/50) or HD (Cat. III/135) number 11- 16 I6 --- HIP Hipparcos (Cat. I/239) number 18- 23 F6.4 mag Hmag Average Hipparcos magnitude 25- 30 F6.4 mag e_Hmag rms uncertainty on mag 32- 35 F4.2 mag Amp Amplitude 37- 52 A16 --- Comm Comments
Byte-by-byte Description of file: table2.dat table3.dat
Bytes Format Units Label Explanations
1- 6 I6 --- HD HD (Cat. III/135) number 7 A1 --- n_HD [*] Note on the variability of the star (1) 9- 14 I6 --- HIP Hipparcos (Cat. I/239) number 16- 22 F7.4 mag Hmag Average Hipparcos magnitude 24- 29 F6.4 mag e_Hmag rms uncertainty on mag 31- 34 F4.2 mag Amp Amplitude 36- 42 F7.5 d Per ? Period
Note (1): *: known ellipsoidal variables and eclipsing binaries
Acknowledgements: Saul J. Adelman
(End) Patricia Bauer [CDS] 29-Jun-1998
| The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line |
© UDS/CNRS