ON THE POSSIBILITY OF SELECTING QUASI-STELLAR GALAXIES FROM BLUE STARS BY OBSERVATIONS IN THE NEAR INFRARED,
Abstract
It is known that a certain fraction of the high-galactic-latitude, faint, blue 'stars' are objects with the same optical properties as the quasi-stellar sources. The possibility of selecting these objects from the white dwarfs by observations in the near infrared is shown. (Author)
Document Details
- Document Type
- Technical Report
- Publication Date
- Jan 01, 1967
- Accession Number
- AD0649853
Entities
People
- Alessandro Braccesi
Organizations
- California Institute of Technology