D. W. Shields Data-verified
Affiliation confirmed via AI analysis of OpenAlex, ORCID, and web sources.
Lecturer
faculty
Research Areas
Links
Biography and Research Information
OverviewAI-generated summary
D. W. Shields' research focuses on astrophysics, specifically investigating the structure and evolution of spiral galaxies. Their work has explored methods for measuring spiral arm pitch angles, as demonstrated in their recent publication "Spirality: A Novel Way to Measure Spiral Arm Pitch Angle." Shields has also contributed to the understanding of star formation within galaxies, examining age gradients in star formation history maps and spatially resolved stellar clusters to provide evidence for density wave theory. Their scholarship includes 16 publications with 29 citations and an h-index of 2. Shields has collaborated with Daniel Kennefick and Julia Kennefick at the University of Arkansas at Fayetteville on multiple publications, as well as with Rafael T. Eufrasio.
Metrics
- h-index: 2
- Publications: 16
- Citations: 29
Selected Publications
-
Evidence in favour of density wave theory through age gradients observed in star formation history maps and spatially resolved stellar clusters (2022)
-
Spirality: A Novel Way to Measure Spiral Arm Pitch Angle (2022)
Collaboration Network
Top Collaborators
- Evidence in favour of density wave theory through age gradients observed in star formation history maps and spatially resolved stellar clusters
- Spirality: A Novel Way to Measure Spiral Arm Pitch Angle
- Evidence in favour of density wave theory through age gradients observed in star formation history maps and spatially resolved stellar clusters
- Spirality: A Novel Way to Measure Spiral Arm Pitch Angle
- Evidence in favour of density wave theory through age gradients observed in star formation history maps and spatially resolved stellar clusters
- Spirality: A Novel Way to Measure Spiral Arm Pitch Angle
- Evidence in favour of density wave theory through age gradients observed in star formation history maps and spatially resolved stellar clusters
- Spirality: A Novel Way to Measure Spiral Arm Pitch Angle
- Evidence in favour of density wave theory through age gradients observed in star formation history maps and spatially resolved stellar clusters
- Spirality: A Novel Way to Measure Spiral Arm Pitch Angle
- Spirality: A Novel Way to Measure Spiral Arm Pitch Angle
- Spirality: A Novel Way to Measure Spiral Arm Pitch Angle
- Spirality: A Novel Way to Measure Spiral Arm Pitch Angle
- Spirality: A Novel Way to Measure Spiral Arm Pitch Angle
- Evidence in favour of density wave theory through age gradients observed in star formation history maps and spatially resolved stellar clusters
- Evidence in favour of density wave theory through age gradients observed in star formation history maps and spatially resolved stellar clusters
- Evidence in favour of density wave theory through age gradients observed in star formation history maps and spatially resolved stellar clusters
- Evidence in favour of density wave theory through age gradients observed in star formation history maps and spatially resolved stellar clusters
Similar Researchers
Based on overlapping research topics