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J/A+A/345/505   UBVI magnitudes of NGC 869 B-type pulsators (Krzesinski+, 1999)

B-type pulsators in the central region of NGC 869 (h Persei) Krzesinski J., Pigulski A., Kolaczkowski Z. <Astron. Astrophys. 345, 505 (1999)> =1999A&A...345..505K
ADC_Keywords: Binaries, eclipsing ; Stars, B-type ; Photometry, UBVRI Keywords: stars: binaries: eclipsing - stars: oscillations - stars: variables: general - Galaxy: open clusters and associations: individual: NGC 869 = h Per Abstract: In the course of the search for B-type pulsators in the central region of h Persei, we discovered two β Cephei stars, Oo692 and Oo992, and one SPB star, Oo893. The first two stars are monoperiodic pulsators with periods of 0.1716946 and 0.1326359 d respectively, and semi-amplitudes smaller than 0.01mag. The light curve of Oo893 can be described by a single 1.193633-day period, slightly non-sinusoidal in shape, and having semi-amplitudes from 19 mmag in I to 48 mmag in U. Oo893 is the first SPB star found in h and χ Persei. In addition, we discovered seven other variables, including three eclipsing binaries and one λ Eri star. One of the binaries is a W UMa-type star and a likely cluster member. We also present new UBV photometry for 258 stars in the field. The average reddening, estimated from the cluster colour-colour diagram, amounts to E(B-V)=0.52mag. A 0.1mag dispersion of reddenings within the cluster is also seen. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table4.dat 105 311 UBV photometry of stars in h Persei curves/* 22 10 Individual UBVI light curves
See also: J/A+A/325/987 : UBV magnitude of NGC 884 B-type pulsators (Krzesinski+ 1997) Byte-by-byte Description of file: table4.dat
Bytes Format Units Label Explanations
1- 5 F5.1 pix Xpos X position (1) 7- 11 F5.1 pix Ypos Y position (1) 13- 16 I4 --- OO ? Oosterhoff (1937AnLei..17a...1O) number (NGC 869 NNNN in Simbad) 18- 20 I3 --- W ? Wildey (1964ApJS....8..439W) number (Cl* NGC 869 W NNNa in Simbad) 21- 22 A2 --- m_W [ab :] Multiplicity index or uncertainty flag on W 24- 28 I5 --- MV ? Moffat & Vogt (1974VeBoc...2....1M) number (Cl* NGC 869 MV NNNNN in Simbad) 29 A1 --- m_MV [ABCD] Multiplicity index on MV 30 A1 --- u_MV Uncertainty flag on MV 32- 37 F6.3 mag Vmag ? V magnitude 39- 43 F5.3 mag B-V ? B-V colour index 45- 47 A3 --- r_B-V Reference to BV photometry (2) 49 A1 --- n_B-V [I] I: BV photometry transformed with the use of I-filter measurements 51- 55 F5.3 mag U-B ? U-B colour index 57 I1 h RAh Right ascension (J2000.0) 59- 60 I2 min RAm Right ascension (J2000.0) 62- 66 F5.2 s RAs Right ascension (J2000.0) 68 A1 --- DE- Declination sign (J2000.0) 69- 70 I2 deg DEd Declination (J2000.0) 72- 73 I2 arcmin DEm Declination (J2000.0) 75- 78 F4.1 arcsec DEs Declination (J2000.0) 80- 94 A15 --- Rem Remarks 96-105 A10 --- VarFile Name of the File containing light curves in subdirectory curves
Note (1): 1pix∼0.15', see figure 1. Note (2): S: star was observed from Suhora only B: star was observed from Bialkow only S+B: star was observed form Suhora and Bialkow
Byte-by-byte Description of file: curves/*
Bytes Format Units Label Explanations
1 A1 --- Filter [UBVI] Filter 3- 14 F12.4 d HJD Heliocentric Julian date 16- 22 F7.4 mag Dmag Differential magnitude in Filter band
Acknowledgements: Andrzej Pigulski History: * 15-Nov-2001: In the light curves (files curves/*) the HJD was corrected following a message by the author (Jurek Krzesinski, ): the HJD had been incorrectly interpretated (too early by 600days) * 28-Feb-2002: the first digit of the Wildey number, omitted, was replaced. * 27-Aug-2002: the multiplicity letter for unresolved multiples was modified: it is now A, B, C, D, according to decreasing brightness (from authors)
(End) Patricia Bauer [CDS] 22-Apr-1999
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

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