Faint blue objects at high galactic latitude II. Palomar Schmidt field centered on selected area 29

Journal Article · Fri Jan 01 00:00:00 EST 1982 · Astrophys. J., Suppl. Ser.; (United States)

DOI:https://doi.org/10.1086/190767· OSTI ID:5527030

Usher, P D; Mattson, D; Warnock, A III

The second part of a list of ultraviolet excess objects is given. The objects have been selected from a Palomer Schmidt field centered on Kapteyn selected area 29. The population of objects belonging to color classes. 1A, 1, and 1B should be comprised primarily of quasars and white dwarfs and should be statistically complete to about B = 18.5 mag. One of the listed objects is a 5 mag optical variable; a journal of observations is given, derived from Harvard archival and contemporary Palomar Schmidt plates.

• Research Organization: Astronomy Department, Pennsylvania State University
• OSTI ID: 5527030
• Journal Information: Astrophys. J., Suppl. Ser.; (United States), Vol. 48:1
• Country of Publication: United States
• Language: English

Related Subjects

71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
BLUE STELLAR OBJECTS
COORDINATES
QUASARS
VARIABLE STARS
WHITE DWARF STARS
ULTRAVIOLET RADIATION
COSMIC RADIO SOURCES
DWARF STARS
ELECTROMAGNETIC RADIATION
RADIATIONS
STARS
640103* - Astrophysics & Cosmology- Quasi-Stellar
Radio
& X-Ray Sources- (-1987)
640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar
Radio & X-Ray Sources