The low dispersion synthetic spectra of cool giant stars
he mean energy distribution of cool giant stars was used for comparison with synthetic spectra. The synthetic spectra was calculated using the various grids of stellar rnodel atrnospheres.
| Hlavní autoři: | , , |
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| Médium: | Článek |
| Jazyk: | English |
| Vydáno: |
Odessa I. I. Mechnykov National University
2017-04-01
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| Edice: | Odessa Astronomical Publications |
| On-line přístup: | http://oap.onu.edu.ua/article/view/98805 |