TH E SHOCK WAVE HEATING MECHANISM OF PULSATING STAR CHROMOSPHERES
A mechanism is suggested which explains the origin and variability of chromospheric emission in the centres of the Mgll h and k lines in the spectra of pulsating stars. According to the model the emission originates from gas heated by a shock wave passing though the outer layers of tie star’s atmosp...
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| Format: | Article |
| Language: | English |
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Odessa I. I. Mechnykov National University
2017-06-01
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| Series: | Odessa Astronomical Publications |
| Online Access: | http://oap.onu.edu.ua/article/view/104672 |