J/AJ/89/1707  Photographic observations of variable stars in M9 (Clement+, 1984)

A new investigation of the variable stars in the globular cluster Messier 9. Clement C.M., Ip P., Robert N. <Astron. J., 89, 1707-1711 (1984)> =1984AJ.....89.1707C 1984AJ.....89.1707C
ADC_Keywords: Clusters, globular ; Stars, variable ; Photometry, photographic Keywords: globular clusters: M9 - stars: variables Abstract: New observations from the southern hemisphere have been used to check the periods for the 11 RR Lyrae variables in and around the globular cluster Messier 9. The periods were determined previously with data from northern observatories where M9 can only be observed over a small range in hour angle. Three of the eleven published periods were found to be in error. As a result of this, the mean period of the RRc variables has been revised from 0.279d to 0.341d, the mean period of the RRab variables has been revised from 0.614d to 0.621d,and a star previously believed to be an RR Lyrae has been reclassified as a Population II Cepheid. One of the RRc variables may be a double-mode pulsator. Another variable was studied, but the data were not sufficient for determining its period. Description: Time-series B photographic photometry for 12 variable stars in the globular cluster M9. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file stars.dat 49 12 List of variables table2.dat 83 50 Time-series B photographic photometry for 12 variable stars in Messier 9 (NGC 6333) -------------------------------------------------------------------------------- See also: J/AJ/101/1352 : Observations of variable stars in M9 (Clement+, 1991) J/AJ/112/618 : CCD photometry of variable stars in M9 (Clement+, 1996) J/AJ/118/453 : M9 RR Lyrae CCD observations (Clement+, 1999) J/MNRAS/434/1220 : Vi light curves of NGC6333 variables (Arellano Ferro+, 2013) Byte-by-byte Description of file: stars.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 A3 --- VName Variable name (VNN), <Cl* NGC 6333 SAW VNN> in Simbad 6- 7 I2 h RAh Simbad Hour of Right Ascension (J2000.0) 9- 10 I2 min RAm Simbad Minute of Right Ascension (J2000.0) 12- 16 F5.2 s RAs Simbad Second of Right Ascension (J2000.0) 18 A1 --- DE- Simbad Sign of the Declination (J2000.0) 19- 20 I2 deg DEd Simbad Degree of Declination (J2000.0) 22- 23 I2 arcmin DEm Simbad Arcminute of Declination (J2000.0) 25- 28 F4.1 arcsec DEs Simbad Arcsecond of Declination (J2000.0) 30- 34 F5.2 mag Bmag Simbad B band magnitude 36- 39 F4.1 mag Vmag ? Simbad V band magnitude 41- 49 F9.7 d Per ? Period (from table3 of the paper) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 F11.3 d HJD Heliocentric Julian day 13- 17 F5.2 mag V1mag B magnitude of V1 19- 23 F5.2 mag V2mag B magnitude of V2 25- 29 F5.2 mag V3mag B magnitude of V3 31- 35 F5.2 mag V4mag B magnitude of V4 37- 41 F5.2 mag V5mag ?=- B magnitude of V5 43- 47 F5.2 mag V6mag ?=- B magnitude of V6 49- 53 F5.2 mag V7mag ?=- B magnitude of V7 55- 59 F5.2 mag V8mag B magnitude of V8 61- 65 F5.2 mag V9mag ?=- B magnitude of V9 67- 71 F5.2 mag V10mag B magnitude of V10 73- 77 F5.2 mag V12mag ?=- B magnitude of V12 79- 83 F5.2 mag V13mag B magnitude of V13 -------------------------------------------------------------------------------- Acknowledgements: Daniel Bramich, ESO, Germany Armando Arellano Ferro, Instituto de Astronomia, UNAM, Mexico
(End) Daniel Bramich [ESO], Patricia Vannier [CDS] 15-Oct-2013
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