circumstellar dust oor Kroaties

circumstellar dust

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cosmic dust
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Variability of more massive (2–8 solar mass) Herbig Ae/Be stars is thought to be due to gas-dust clumps, orbiting in the circumstellar disks.
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We have determined the physical properties of circumstellar dust in different obscuration intervals and in different stages after the nova outburst, with special emphasis on two probably best observed symbiotic Miras, HM Sge and RR Tel.
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To understand such symbiotic Miras, their evolution, mutual interactions between the components and circumstellar matter, the influence of stellar winds and mass transfer mechanism, it is essential to determine the properties of circumstellar dust and their temporal evolution.
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Spectroscopic and photometric investigation of stars in various evolutionary phases is focused on circumstellar envelopes that consist of gas and dust.
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