A NEW METHOD TO ESTIMATE LOCAL PITCH ANGLES IN SPIRAL GALAXIES: APPLICATION TO SPIRAL ARMS AND FEATHERS IN M81 AND M51
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/1538-3881/148/i=6/a=133/pdf
Reference70 articles.
1. Local interstellar gasdynamical stability and substructure in spiral arms
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5. Macromolecules, Very Small Grains, and Large Dust Particles in the Whirlpool Galaxy M51 and Its Companion: A Unified View
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1. Morphology and Kinematics of the Gas in M51: How Interaction with NGC 5195 Has Molded the Structure of Its Arms;The Astrophysical Journal;2024-04-29
2. Galaxies decomposition with spiral arms – II. A multiwavelength case study of M 51;Monthly Notices of the Royal Astronomical Society;2024-01-11
3. Colour jumps across the spiral arms of Hubble Ultra Deep Field galaxies;Monthly Notices of the Royal Astronomical Society;2023-06-16
4. Spirality: A Novel Way to Measure Spiral Arm Pitch Angle;Galaxies;2022-10-17
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