QSO Emission Line Redshift Differences

Symposium - International Astronomical Union
doi 10.1017/s0074180900140586
Full Text
Abstract

Available in full text

Date
Authors
Publisher

Cambridge University Press (CUP)

Related search

X-Ray Insights Into the Nature of Weak Emission-Line Quasars at High Redshift

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2009English

Galaxy Evolution From QSO Absorption-Line Selected Samples

Symposium - International Astronomical Union
1996English

Hα Emission Lines in High Redshift Quasars

Symposium - International Astronomical Union
1989English

350 Micron Dust Emission From High-Redshift Objects

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
1999English

PKS 0537-441: Extended [O II] Emission and a Binary QSO?

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2003English

The Metal Absorption Systems of the QSO 0103-260 and the Galaxy Redshift Distribution in the FORS Deep Field

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2003English

Quasar Emission - Line Strengths

Symposium - International Astronomical Union
1989English

A Tight Relation Between N/O Ratio and Galaxy Stellar Mass Can Explain the Evolution of Strong Emission Line Ratios With Redshift

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2016English

Quasar Emission Line Profile Modelling

Symposium - International Astronomical Union
1989English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2025 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy