Uplift, Feedback, and Buoyancy: Radio Lobe Dynamics in NGC 4472-Reference-Cited by-同舟云学术

Uplift, Feedback, and Buoyancy: Radio Lobe Dynamics in NGC 4472

Published:2017-10-09 Issue:1 Volume:848 Page:26
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Gendron-Marsolais M.^ORCID,Kraft R. P.^ORCID,Bogdan A.,Hlavacek-Larrondo J.^ORCID,Forman W. R.^ORCID,Jones C.,Su Y.,Nulsen P.^ORCID,Randall S. W.^ORCID,Roediger E.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/848/i=1/a=26/pdf

Reference59 articles.

1. Abundances of the elements: Meteoritic and solar

2. THE UNUSUAL X-RAY MORPHOLOGY OF NGC 4636 REVEALED BY DEEPCHANDRAOBSERVATIONS: CAVITIES AND SHOCKS CREATED BY PAST ACTIVE GALACTIC NUCLEUS OUTBURSTS

3. Hot Gas Structure in the Elliptical Galaxy NGC 4472

4. A Systematic Study of Radio‐induced X‐Ray Cavities in Clusters, Groups, and Galaxies

5. THE ACS FORNAX CLUSTER SURVEY. V. MEASUREMENT AND RECALIBRATION OF SURFACE BRIGHTNESS FLUCTUATIONS AND A PRECISE VALUE OF THE FORNAX-VIRGO RELATIVE DISTANCE

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