Published December 1986
| Version v1
Journal article
Do density waves trigger star formation?
Creators
- 1. IBM Thomas J. Watson Research Center, Yorktown Heights, NY
Description
A comparison of B - V colors, blue and far-IR surface brightnesses, metallicities, and star formation rates calculated from H-alpha and UV fluxes reveals no difference in the average star formation rates for galaxies with and without grand design spiral structure. This implies that strong density waves do not trigger a significant excess of star formation compared to that in similar galaxies without a wave. Density waves organize the gas and young stars into spiral arms because of the flow pattern, and they may influence the formation and destruction of the largest cloud complexes, but they appear to contribute less than 50 percent to the overall star formation rate. 46 references
Additional details
Publishing Information
- Journal Title
- Astrophys. J.
- Journal Volume
- 311
- Series
- Astrophys. J.
- Journal Page Range
- 554-562
- ISSN
- 0004-637X
- CODEN
- ASJOA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 18078174
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BALMER LINES; COSMIC GASES; GALACTIC EVOLUTION; GALAXIES; LUMINOSITY; MORPHOLOGICAL CHANGES; SPIRAL CONFIGURATION; STAR EVOLUTION; ULTRAVIOLET RADIATION
- Descriptors DEC
- CONFIGURATION; ELECTROMAGNETIC RADIATION; FLUIDS; GASES; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; RADIATIONS