Barbara Ryden

From Wikipedia, the free encyclopedia
Barbara Sue Ryden Pogge
Alma materNorthwestern University
Princeton University
Scientific career
InstitutionsOhio State University
Harvard–Smithsonian Center for Astrophysics
Canadian Institute for Theoretical Astrophysics
ThesisGalaxy formation by gravitational collapse in a universe dominated by cold dark matter (1987)
InfluencedAlberto Conti

Barbara Sue Ryden (born May 2, 1961) is an American astrophysicist who is a Professor of Astronomy at Ohio State University. Her research considers the formation, shape and structure of galaxies. She was elected a fellow of the American Association for the Advancement of Science in 2016.

Early life and education[]

Ryden studied physics and integrated sciences at Northwestern University.[1] She moved to Princeton University as a doctoral student, where she worked alongside James Gunn.[2] She was a postdoctoral research fellow at the Harvard–Smithsonian Center for Astrophysics and Canadian Institute for Theoretical Astrophysics.[citation needed]

Research and career[]

Ryden joined the faculty at Ohio State University in 1992. She studies the formation and shapes of galaxies.[3][4] Her research made use of the Sloan Digital Sky Survey and various numerical simulations.[5] She has shown that the galactic disks at the centre of spiral galaxies are more elliptical than circular.[6]

Ryden has written several astronomy textbooks, including Introduction to Cosmology, Interstellar and Intergalactic Medium and Foundations of Astrophysics.[citation needed]

Awards and honors[]

Selected publications[]

  • Barbara S. Ryden; James E. Gunn (July' '1987). "Galaxy formation by gravitational collapse". The Astrophysical Journal. 318: 15. Bibcode:1987ApJ...318...15R. doi:10.1086/165349. ISSN 0004-637X. Wikidata Q105030634. Check date values in: |publication-date= (help)
  • William H. Press; Barbara S. Ryden; David N. Spergel (December' '1989). "Dynamical evolution of domain walls in an expanding universe". The Astrophysical Journal. 347: 590. Bibcode:1989ApJ...347..590P. doi:10.1086/168151. ISSN 0004-637X. Wikidata Q105030622. Check date values in: |publication-date= (help)
  • Press WH; Barbara Ryden; Spergel DN (1' 'March' '1990). "Single mechanism for generating large-scale structure and providing dark missing matter". Physical Review Letters. 64 (10): 1084–1087. Bibcode:1990PhRvL..64.1084P. doi:10.1103/PHYSREVLETT.64.1084. ISSN 0031-9007. PMID 10041295. Wikidata Q74499882. Check date values in: |publication-date= (help)

Books[]

References[]

  1. ^ "Inspire". inspirehep.net. Retrieved 2021-01-22.
  2. ^ Barbara Sue Ryden (1987), Galaxy formation by gravitational collapse in a universe dominated by cold dark matter, Bibcode:1987PhDT.........2R, OCLC 946084398, Wikidata Q105201377
  3. ^ "Barbara Ryden". astronomy.osu.edu. Retrieved 2021-01-22.
  4. ^ Barbara Ryden (March' '2017). "A constant conflict". Nature Physics. 13 (3): 314–314. Bibcode:2017NatPh..13..314R. doi:10.1038/NPHYS4055. ISSN 1745-2473. Wikidata Q105199593. Check date values in: |publication-date= (help)
  5. ^ Cayman T. Unterborn; Barbara S. Ryden (10' 'November' '2008). "Inclination‐Dependent Extinction Effects in Disk Galaxies in the Sloan Digital Sky Survey". The Astrophysical Journal. 687 (2): 976–985. arXiv:0801.2400. Bibcode:2008ApJ...687..976U. doi:10.1086/591898. ISSN 0004-637X. Wikidata Q60735035. Check date values in: |publication-date= (help)
  6. ^ Ryden B. S. (2004). "The ellipticity of the disks of spiral galaxies". Letters of the Astrophysical Journal. 601: 214–220. arXiv:astro-ph/0310097. Bibcode:2004ApJ...601..214R. doi:10.1086/380437. ISSN 2041-8205. Wikidata Q68886977.
  7. ^ "3 Young Researchers Receive National Award". 3 Young Researchers Receive National Award. Retrieved 2021-01-22.
  8. ^ "Chambliss Astronomical Writing Award | American Astronomical Society". aas.org. Retrieved 2021-01-22.
  9. ^ "2016 Fellows | American Association for the Advancement of Science". www.aaas.org. Retrieved 2021-01-22.
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