Skip to main navigation
Skip to search
Skip to main content
University of Hertfordshire (Research Profiles) Home
Search content at University of Hertfordshire (Research Profiles)
Home
Profiles
Research output
Projects
Research units
Using
26
Al to detect ongoing self-enrichment in young massive star clusters
Katarzyna Nowak
,
Martin G. H. Krause
, Thomas Siegert
,
Jan Forbrich
,
Robert M. Yates
, Laura Ramírez-Galeano
, Corinne Charbonnel
, Mark Gieles
School of Physics, Engineering & Computer Science
Department of Physics, Astronomy and Mathematics
Centre for Astrophysics Research (CAR)
Research output
:
Contribution to journal
›
Article
›
peer-review
25
Downloads (Pure)
Overview
Fingerprint
Fingerprint
Dive into the research topics of 'Using
26
Al to detect ongoing self-enrichment in young massive star clusters'. Together they form a unique fingerprint.
Sort by
Weight
Alphabetically
Keyphrases
Massive Stars
100%
Star Clusters
100%
Self-enhancement
100%
26Al
100%
Detection Method
28%
Globular Clusters
28%
Polluter
28%
Compton Spectrometer
28%
Compton Imager
28%
Atacama Large Millimeter/submillimeter Array
28%
Radio Recombination Lines
14%
Chemical Composition
14%
Square Kilometre Array
14%
Nearby Galaxies
14%
Large Magellanic Cloud
14%
Target Monitoring
14%
Radioactive Decay
14%
Decay Products
14%
Enrichment Method
14%
Positronium
14%
Gamma-ray Data
14%
Enrichment Clusters
14%
Gasses
14%
Major Challenges
14%
Chemical Anomaly
14%
Earth and Planetary Sciences
Massive Star
100%
Star Cloud
100%
Detection Method
40%
Magellanic Clouds
20%
Decay Product
20%
Positronium
20%
Gamma Radiation
20%
Radioactivity
20%
Physics
Massive Star
100%
Star Cluster
100%
Globular Cluster
40%
Gamma Radiation
20%
Large Magellanic Cloud
20%
Positronium
20%
Radioactivity
20%