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

Abstract

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.

Authors:
; ;
Publication Date:
Research Org.:
Astronomy Department, Pennsylvania State University
OSTI Identifier:
5527030
Resource Type:
Journal Article
Journal Name:
Astrophys. J., Suppl. Ser.; (United States)
Additional Journal Information:
Journal Volume: 48:1
Country of Publication:
United States
Language:
English
Subject:
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

Citation Formats

Usher, P D, Mattson, D, and Warnock, A III. Faint blue objects at high galactic latitude II. Palomar Schmidt field centered on selected area 29. United States: N. p., 1982. Web. doi:10.1086/190767.
Usher, P D, Mattson, D, & Warnock, A III. Faint blue objects at high galactic latitude II. Palomar Schmidt field centered on selected area 29. United States. https://doi.org/10.1086/190767
Usher, P D, Mattson, D, and Warnock, A III. 1982. "Faint blue objects at high galactic latitude II. Palomar Schmidt field centered on selected area 29". United States. https://doi.org/10.1086/190767.
@article{osti_5527030,
title = {Faint blue objects at high galactic latitude II. Palomar Schmidt field centered on selected area 29},
author = {Usher, P D and Mattson, D and Warnock, A III},
abstractNote = {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.},
doi = {10.1086/190767},
url = {https://www.osti.gov/biblio/5527030}, journal = {Astrophys. J., Suppl. Ser.; (United States)},
number = ,
volume = 48:1,
place = {United States},
year = {Fri Jan 01 00:00:00 EST 1982},
month = {Fri Jan 01 00:00:00 EST 1982}
}