The most distant [O III]-emitting quasar PKS 1937-101 at redshift 3.8

Yoshiaki Taniguchi, Takashi Murayama, Kimiaki Kawara, Nobuo Arimoto

Research output: Contribution to journalArticlepeer-review

6 Citations (Scopus)

Abstract

We report on the discovery of a high-z quasar with unambiguous [O III]λ5007 emission: PKS 1937-101 at redshift 3.8. This quasar, however, shows little evidence for rest-frame ultraviolet and optical Fe II emission. It is thus shown that PKS 1937-101 does not belong to a class of super-iron-rich high-z quasars reported by Elston, Thompson, and Hill (1994, AAA61.159.045). The epoch of major star formation in the host galaxy is briefly discussed.

Original languageEnglish
Pages (from-to)419-424
Number of pages6
JournalPublications of the Astronomical Society of Japan
Volume49
Issue number4
DOIs
Publication statusPublished - 1997

Keywords

  • Cosmology: observations
  • Galaxies: evolution
  • Galaxies: formation
  • Quasars: emission lines
  • Quasars: individual (PKS 1937-101)

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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