J/ApJS/98/659               Galactic PNe statistical distance scale (Zhang 1995)

A statistical distance scale for galactic planetary nebulae Zhang C.Y. <Astrophys. J. Suppl. Ser. 98, 659 (1995)> =1995ApJS...98..659Z 1995ApJS...98..659Z
ADC_Keywords: Planetary nebulae ; Stars, distances Keywords: distance scale - planetary nebulae: general Description: A statistical distance scale is proposed. It is based on the correlation between the ionized mass and the radius and the correlation between the radio continuum surface brightness temperature and the nebular radius. The proposed statistical distance scale is an average of the two distances obtained using the correlations. These correlations, calibrated on the 132 planetary nebulae with well-determined individual distances by Zhang, can reproduce not only the average distance of a sample of Galactic Bulge planetary nebulae exactly at the distance to the Galactic center, but also the expected gaussian distribution of their distances around the Galactic center. This new distance scale is applied to 647 Galactic planetary nebulae. It is estimated that this distance scale can be accurate on average to 35%-50%. Our statistical distance scale is in good agreement with the one recently proposed by Van de Steene and Zijlstra File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1 78 134 Planetary nebulae with individually determined distances table1.tex 113 159 LaTeX version of table1 table3 72 647 Catalog of statistical distances of planetary nebulae table3.tex 100 675 LaTeX version of table3 -------------------------------------------------------------------------------- See also: V/84 : Strasbourg-ESO Catalogue of Galactic Planetary Nebulae (Acker+ 1992) Byte-by-byte Description of file: table1 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 A7 --- Name Common name 9- 16 A8 --- PK Perek & Kohoutek name 18- 22 F5.2 kpc Dist Individually determined distance 24- 27 I4 mJy S5GHz 5 GHz (6 cm) radio flux density 29- 33 F5.1 arcsec Diam Diameter of nebula 35- 41 F7.2 K Tb Radio Brightness Temperature 43- 47 F5.3 pc Rad Radius of nebula 49- 54 E6.1 solMass Mi Ionized gas mass of nebula 56- 60 F5.2 kpc DMi Statistical distance derived from mass-radius relation 62- 66 F5.2 kpc DTb Statistical distance from Tb - R relation 68- 72 F5.2 kpc Df Mean of DMi and DTb adopted as final result (1) 74- 78 F5.1 % Delta ? Fractional difference between Df and Dist -------------------------------------------------------------------------------- Note (1): In Table 1 of the paper, Dm should read Df. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name Common name 11- 18 A8 --- PK PK name 19- 24 F6.1 mJy S5GHz 5 GHz (6 cm) radio flux density 26- 30 F5.1 arcsec Diam Diameter of nebula in arcsec 32- 34 I3 --- Ref References for the previous columns (1) 36- 42 F7.2 K Tb Radio Brightness Temperature 44- 48 F5.2 kpc DMi Statistical distance derived from mass-radius relation 50- 54 F5.2 kpc DTb Statistical distance from Tb - R relation 56- 60 F5.2 kpc Df Mean of DMi and DTb adopted as final result (2) 62- 66 F5.2 kpc D(VSZ) ? Distance from Van de Steene and Zijstra (1995) 68- 72 F5.2 kpc D(CKS) ? Distance from Cahn, Kaler & Stanghellini (1992) -------------------------------------------------------------------------------- Note (1): Reference numbers are: 1: Pottasch (1994A&A...289..261P 1994A&A...289..261P) 2: Aaquist & Kwok (1990A&AS...84..229A 1990A&AS...84..229A) 3: Zijlstra et al. (1989A&AS...79..329Z 1989A&AS...79..329Z) 4: Milne & Aller (1975A&A....38..183M 1975A&A....38..183M) 5: Milne (1979A&AS...36..227M 1979A&AS...36..227M) 6: Roelfsema et al. (1991A&A...251..611R 1991A&A...251..611R) 7: Cahn et al. (1992A&AS...94..399C 1992A&AS...94..399C) 8: Pottasch & Zijlstra (1994A&A...289..261P 1994A&A...289..261P) Note (2): In Table 3 of the paper, Dm should read Df. -------------------------------------------------------------------------------- Acknowledgements: References: Aaquist & Kwok, 1990 A&AS 84, 229 =1990A&AS...84..229A 1990A&AS...84..229A Cahn et al., 1992 A&AS 94, 399 =1992A&AS...94..399C 1992A&AS...94..399C Milne, 1979 A&AS 36, 227 =1979A&AS...36..227M 1979A&AS...36..227M Milne & Aller, 1975 A&A 38, 183 =1975A&A....38..183M 1975A&A....38..183M Pottasch, 1984 Planetary nebulae (Dordrecht: Reidel) Pottasch & Zijlstra, 1994 A&A 289, 261 =1994A&A...289..261P 1994A&A...289..261P Roelfsema et al., 1991 A&A 251, 611 =1991A&A...251..611R 1991A&A...251..611R Van de Steene and Zijlstra, 1994, =1994A&AS..108..485V 1994A&AS..108..485V Van de Steene and Zijlstra, 1995, A&A 293, 541 =1995A&A...293..541V 1995A&A...293..541V Zijlstra et al., 1989 A&AS 79, 329 =1989A&AS...79..329Z 1989A&AS...79..329Z
(End) Patricia Bauer [CDS] 28-Aug-1996
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