J/A+AS/123/115      Variables stars in Palomar-Groningen field 3 (Ng+ 1997)

Field 3 of the Palomar-Groningen Survey. I. Variable stars at the edge of the Sagittarius dwarf galaxy Ng Y.K., Schultheis M. <Astron. Astrophys. Suppl. Ser. 123, 115 (1997)> =1997A&AS..123..115N 1997A&AS..123..115N (SIMBAD/NED BibCode)
ADC_Keywords: Stars, variable ; Magnitudes, photographic Keywords: stars: carbon ; AGB, post-AGB; variables: others - Local Group - galaxies: Sagittarius dwarf Abstract: A catalogue is presented with variable (RR Lyrae, semiregular and Mira) stars located inside field #3 (PG3) of the Palomar-Groningen Survey at the outer edge of the Sagittarius dwarf galaxy. One of the semiregular variables is a carbon star, comparable with those found by Azzopardi et al. (1991A&AS...88..265A 1991A&AS...88..265A). Serendipity provides the suggestion, that their carbon stars might not be located inside, but behind the bulge on the Sagittarius dwarf galaxy. Objects: -------------------------------------------------- RA (2000) DE Designation(s) -------------------------------------------------- 19 29 58.9 -17 40 40 Sagittarius dwarf galaxy -------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1 77 22 Catalogue of PG3 variable stars find_pg3.ps 1023 23098 Finding charts -------------------------------------------------------------------------------- See also: J/A+A/338/581 : Field 3 Palomar-Groningen survey. II. (Schultheis+ 1998) Byte-by-byte Description of file: table1 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 --- ID Star number (1) 6- 13 A8 --- VarType Variable type (2) 16- 17 I2 h RAh Right ascension (J2000) 19- 20 I2 min RAm Right ascension (J2000) 22- 25 F4.1 s RAs Right ascension (J2000) 27 A1 --- DE- Declination sign 28- 29 I2 deg DEd Declination (J2000) 31- 32 I2 arcmin DEm Declination (J2000) 34- 37 F4.1 arcsec DEs Declination (J2000) 40- 44 F5.1 deg GLON Galactic longitude 46- 50 F5.1 deg GLAT Galactic latitude 53- 57 F5.2 mag Bmag Mean photographic BJ magnitude (3) 59- 63 F5.2 mag Rmag Mean photographic RF magnitude (3) 66- 75 F10.6 d P ? Period 77 I1 --- Q [0/3] Quality flag (4) -------------------------------------------------------------------------------- Note (1): Variable star number, following Plaut (1971A&AS....4...75P 1971A&AS....4...75P) and Wesselink (1987) Note (2): Variable star classification, where the semiregular classification is taken from Plaut (1971A&AS....4...75P 1971A&AS....4...75P); if two classifications are given, the first is from Wesselink (1987) and the second from Plaut (1971A&AS....4...75P 1971A&AS....4...75P) Note (3): The mean B_J and R_F photographic magnitudes for the RR Lyrae and the Mira are from Wesselink (1987). The photographic photometry of the semiregular variables is obtained in the study by Ng (1994) Note (4): Quality flag (classification and period) of variable star following Wesselink (1987); Q=0: no doubt about the determined period and classification, Q=1: classification is correct but alternative period is possible, Q=2: period determination is correct but the classification is doubtful, Q=3: both period determination and classification are unreliable -------------------------------------------------------------------------------- Acknowledgements: Yuen Keong Ng References: Ng Y.K., 1994, Ph.D. thesis, Leiden University, the Netherlands Plaut L., 1971, A&AS 4, 75 Wesselink Th.J.H., 1987, Ph.D. thesis, Catholic University Nijmegen, the Netherlands
(End) Patricia Bauer [CDS] 13-Jan-1997
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