Offsets between Hα and CO Arms of a Spiral Galaxy, NGC 4254: A New Method for Determining the Pattern Speed of Spiral Galaxies
- 25 December 2004
- journal article
- Published by Oxford University Press (OUP) in Publications of the Astronomical Society of Japan
- Vol. 56 (6) , L45-L48
- https://doi.org/10.1093/pasj/56.6.l45
Abstract
No abstract availableAll Related Versions
This publication has 18 references indexed in Scilit:
- Probing for Dark Matter within Spiral Galaxy DisksThe Astrophysical Journal, 2001
- An Atlas of Hα and R Images and Radial Profiles of 63 Bright Virgo Cluster Spiral GalaxiesThe Astrophysical Journal Supplement Series, 2001
- Tracing the Dynamics of Disk Galaxies with Optical and Infrared Surface Photometry: Color Gradients in M99The Astrophysical Journal, 1996
- HI in M81. I. Large Scale Structure and Spiral Density WavesThe Astronomical Journal, 1996
- NGC 4254: A Spiral Galaxy with an M = 1 Mode and Infalling GasThe Astrophysical Journal, 1993
- A new way to locate corotation resonances in spiral galaxiesThe Astrophysical Journal, 1993
- Star Formation Triggering by Density Waves in the Grand Design Spirals NGC 3992 and NGC 628The Astrophysical Journal, 1990
- Arm classifications for spiral galaxiesThe Astrophysical Journal, 1987
- Spectral analysis of the asymmetric spiral pattern of NGC 4254The Astrophysical Journal, 1982
- On the Spiral Structure of Disk Galaxies.The Astrophysical Journal, 1964