/ftp/cats/J/A%2BA/364/712



==========================================================================
J/A+A/364/712       BV photometry in Draco molecular cloud   (Penprase+, 2000)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	table5.dat table6.dat
==========================================================================
Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A+A/364/712
==========================================================================

drwxr-xr-x 12 cats archive 216 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 480 Dec 19 2022 .message -r--r--r-- 1 cats archive 4714 Jul 25 2001 ReadMe -rw-r--r-- 1 cats archive 1008 Nov 13 2012 +footg5.gif -rw-r--r-- 1 cats archive 2511 Nov 13 2012 +footg8.gif -r--r--r-- 1 cats archive 6849 Jul 25 2001 table5.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 1893 Jul 14 2001 table6.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+A/364/712 BV photometry in Draco molecular cloud (Penprase+, 2000) ================================================================================ Optical observations of the Draco molecular cloud. I. Catalog of B and V magnitudes for selected areas. Penprase B.E., Rhodes J.D., Harris E.L. <Astron. Astrophys. 364, 712 (2000)> =2000A&A...364..712P ================================================================================ ADC_Keywords: Molecular clouds ; Photometry, UBV Keywords: ISM: clouds - ISM: dust, extinction - ISM: general - ISM: structure - Galaxy: halo - techniques: photometric Description: To investigate the distance and linear dimensions of the Draco Molecular Cloud (MBM 41) we have obtained new CCD photometry for a selection of stars in 20 selected areas toward the cores of the cloud. The selected areas were chosen to coincide with the brightest IRAS emitting portions of the cloud, and also with dense ^12^CO emission from the cloud. For each area we have obtained V and B photometry, and a subset of the fields has also been observed through a narrow-band Halpha filter and in the U band. We present V and B magnitudes for the 362 stars which have high-quality observations in both bands. The observations were made during the nights of June 29 and June 30, 1993 at the Palomar Observatory, using the 1.5-meter telescope and Palomar 6 Tektronix CCD camera with 24 micron pixels.