The study of observations on the RT-22 Krao maser sources in the line of water vapor at a wavelength of 1.35 cm
Heading:
| 1Volvach, AE, 2Shulga, VM, 1Strepka, ID, 2Antyufeev, AV, 3Myshenko, VV, 1Volvach, LN 1Laboratory of Radio Astronomy, SRI Crimean Astrophysical Observatory, Katsiveli, AR Crimea, Ukraine 2Institute of Radio Astronomy, National Academy of Sciences of Ukraine, Kharkiv, Ukraine 3Institute of Radio Astronomy of the National Academy of Sciences of Ukraine, Kharkiv, Ukraine |
| Kosm. nauka tehnol. 2002, 8 ;(Supplement2):289-292 |
| https://doi.org/10.15407/knit2002.02s.289 |
| Publication Language: Russian |
Abstract: For systematic and complex studies of the star formation regions, a 15-kHz frequency resolution receiver based on PC-MARK-CAMAC for spectral-polarimetric observations of maser sources in the water vapor line was developed and put into operation. Commissioning the Fourier spectrum analyzer significantly increases the frequency resolution. In the single antenna mode, spectral observations of the Orion KL maser radiation source were carried out. The measured antenna temperatures in the lines correspond to the calm state of the object.
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