Uncovering Spiral Structure in Flocculent Galaxies

@article{Thornley1996UncoveringSS,
  title={Uncovering Spiral Structure in Flocculent Galaxies},
  author={Michele D. Thornley},
  journal={The Astrophysical Journal Letters},
  year={1996},
  volume={469},
  pages={L45 - L48}
}
  • M. Thornley
  • Published 7 July 1996
  • Physics
  • The Astrophysical Journal Letters
We present K' (2.1 μm) observations of four nearby flocculent spirals, which clearly show low-level spiral structure and suggest that kiloparsec-scale spiral structure is more prevalent in flocculent spirals than previously supposed. In particular, the prototypical flocculent spiral NGC 5055 is shown to have regular, two-arm spiral structure to a radius of 4.0 kpc in the near-infrared, with an arm-interarm contrast of 1.3. The spiral structure in all four galaxies is weaker than that in grand… 
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