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http://arxiv.org/pdf/astro-ph/...
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arXiv.org e-Print Archive
Preprint . 1997
Data sources: arXiv.org e-Print Archive
https://doi.org/10.1007/978-3-...
Part of book or chapter of book . 1997 . Peer-reviewed
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https://dx.doi.org/10.48550/ar...
Article . 1997
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https://dx.doi.org/10.1007/978...
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Observing the Galaxy Environment of QSOs

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Article , Preprint , Other literature type 01 Jan 1997Embargo end date: 01 Jan 1997Publisher:Springer Berlin Heidelberg
Authors: J\\"ager, Klaus; Fricke, Klaus J.; Heidt, Jochen;

doi: 10.1007/978-3-540-69648-3_16 , 10.48550/arxiv.astro-ph/9702175

arXiv: astro-ph/9702175

Observing the Galaxy Environment of QSOs

Abstract

2 pages, 1 figure (postscript), Latex (uses lamuphys.sty). To appear in the proceedings of the ESO/IAC Conference on 'Quasar Hosts' held in Puerta de la Cruz, Tenerife, Spain, Sep. 24-27 1996

We outline our recently started program to investigate the galaxy environment of QSOs, in particular of radio-quiet objects at intermediate redshifts.

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Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
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