We present observations of Venus at six frequencies: 1.385, 1.465, 4.86, 8.44, 14.94, and 22.46 GHz. These were obtained with the Very Large Array and calibrated in a consistent fashion. The brightness temperature of Venus at the six frequencies is derived and compared to a model which includes the
New observations of ULX supershells, and their implications
β Scribed by D.M. Russell; Y.-J. Yang; J.C. Gladstone; K. Wiersema; T.P. Roberts
- Publisher
- John Wiley and Sons
- Year
- 2011
- Tongue
- English
- Weight
- 154 KB
- Volume
- 332
- Category
- Article
- ISSN
- 0004-6337
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