New Photometric Data of Old Open Clusters in the Anti-Galactic Center Region

[1]  K. Janes,et al.  Open clusters and galactic structure. , 1982 .

[2]  T. Hawarden Mass loss from red giants in old open clusters , 1975 .

[3]  R. Trumpler Preliminary results on the distances, dimensions and space distribution of open star clusters , 1930 .

[4]  G. Rieke,et al.  The interstellar extinction law from 1 to 13 microns. , 1985 .

[5]  B. Anthony-Twarog,et al.  Faint stellar photometry in clusters. II. NGC 6791 and NGC 6535. , 1985 .

[6]  Michael J. West,et al.  The globular cluster system of the Galaxy. III: measurements of radial velocity and metallicity for 60 clusters and a compilation of metallicities for 121 clusters , 1984 .

[7]  V. Castellani,et al.  The evolution through H and He burning of Galactic cluster stars , 1992 .

[8]  Setting the Clock of Stellar Models , 1992 .

[9]  When and why is the random force in Brownian motion a Gaussian process. , 1991, Biophysical chemistry.

[10]  R. Cannon Red giants in old open clusters. , 1970 .

[11]  J. Mathis,et al.  The relationship between infrared, optical, and ultraviolet extinction , 1989 .

[12]  P. Stetson DAOPHOT: A COMPUTER PROGRAM FOR CROWDED-FIELD STELLAR PHOTOMETRY , 1987 .

[13]  S. Okamura,et al.  Large-scale structure of galaxies in the Ophiuchus region , 2000 .

[14]  Randy L. Phelps,et al.  Development of the Galactic Disk: A Search for the Oldest Open Cluster , 1994 .

[15]  J. Kaluzny CCD photometry of distant open clusters - IV. Trumpler 5 , 1998 .

[16]  R. Phelps Berkeley 17: The Oldest Open Cluster? , 1997 .

[17]  James Liebert,et al.  The Age, Extinction, and Distance of the Old, Metal-rich Open Cluster NGC 6791 , 1998, astro-ph/9812097.

[18]  K. Ashman,et al.  Some Revised Observational Constraints on the Formation and Evolution of the Galactic Disk , 1997, astro-ph/9709122.

[19]  J. Clariá,et al.  Chemical Evolution of the Galactic Disk: Evidence for a Gradient Perpendicular to the Galactic Plane , 1995 .

[20]  E. D. Friel,et al.  The Old Open Clusters of the Milky Way , 1995 .

[21]  S. Seltzer Future trends in endodontics , 1993 .

[22]  Brian H. Houston,et al.  Fiber-optic air-backed hydrophone transduction mechanisms , 1991 .

[23]  G. Carraro,et al.  On the Galactic disc age–metallicity relation , 1998 .

[24]  V. Kozhurina-Platais,et al.  WIYN Open Cluster Study. II. UBVRI CCD Photometry of the Open Cluster NGC 188 , 1999 .

[25]  L. Spitzer Distribution of Galactic Clusters. , 1958 .

[26]  Arlo U. Landolt,et al.  UBVRI Photometric Standard Stars in the Magnitude Range 11 , 1992 .

[27]  D. VandenBerg Evolution of 0. 7--3. 0 M/sub sun/ stars having -1. 0< or =(Fe/H)< or =0. 0 , 1985 .

[28]  M. Pinsonneault,et al.  The ages of the disk clusters NGC 188, M67, and NGC 752, using improved opacities and cluster membership data , 1995 .

[29]  Giovanni Carraro,et al.  IS THE GALACTIC DISC OLDER THAN THE HALO , 1999 .

[30]  K. Janes,et al.  The Galactic System of Old Star Clusters: The Development of the Galactic Disk , 1994 .

[31]  H. Guetter Photometric Study of the Old Galactic Cluster Be 31 , 1993 .