No CrossRef data available.
Article contents
Radio Observations of Hii Regions in M33
Published online by Cambridge University Press: 14 August 2015
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
The Westerbork Synthesis Radio Telescope was used to map the continuum radiation of M33 at 1415 MHz. Of 67 radio sources with fluxes S> 1.8 mJy (3σ), 60% coincide with Hα sources. These are all intrinsically stronger than 4 × the Orion nebula, i.e., they are giant Hiiregions. The two strongest sources, NGC 604 (58 mJy) and NGC 595 (20 mJy), are similar to W51.
- Type
- Part 2: Galactic H ii Regions
- Information
- Symposium - International Astronomical Union , Volume 60: Galactic Radio Astronomy , 1974 , pp. 227 - 228
- Copyright
- Copyright © Reidel 1974
You have
Access