Skip to main navigation
Skip to search
Skip to main content
The Hebrew University of Jerusalem Home
Approve / Request updates on publications
Home
Profiles
Research units
Research output
Prizes
Search by expertise, name or affiliation
Galaxy bimodality due to cold flows and shock heating
Avishai Dekel
*
,
Yuval Birnboim
*
Corresponding author for this work
Racah Institute of Physics
Research output
:
Contribution to journal
›
Article
›
peer-review
1482
Scopus citations
Overview
Fingerprint
Fingerprint
Dive into the research topics of 'Galaxy bimodality due to cold flows and shock heating'. Together they form a unique fingerprint.
Sort by
Weight
Alphabetically
Keyphrases
Galaxies
100%
Shock Heating
100%
Cold Flow
100%
Bimodality
100%
Cold Shock
100%
Flow Heating
100%
Halo
75%
Shock
50%
Virion
50%
Star Formation
50%
Massive Galaxies
50%
Starburst
50%
Gasses
50%
Supernovae
25%
Long Sequence
25%
Stellar Masses
25%
Feedback Processes
25%
Active Galactic nuclei
25%
Dark Matter Halos
25%
Star-forming
25%
Star Formation History
25%
Truncation
25%
Angular Momentum
25%
Clustering Process
25%
Characteristic Scale
25%
Thermal Properties
25%
Qualitative Features
25%
Feedback Capacity
25%
Gas Supply
25%
Galaxy Properties
25%
Color-magnitude
25%
Magnitude Information
25%
Physics
Star Formation
100%
Shock Heating
100%
Energetics
33%
Supernovae
33%
Stellar Mass
33%
Dark Matter
33%
Angular Momentum
33%
Active Galactic Nuclei
33%
Galaxy Properties
33%
L Galaxies
33%
Early Star
33%