Результаты исследований: Научные публикации в периодических изданиях › Обзорная статья › Рецензирование
Scattered Radiation of Protoplanetary Disks. / Grinin, Vladimir P.; Tambovtseva, Larisa V.
в: Universe, Том 8, № 4, 224, 01.04.2022.Результаты исследований: Научные публикации в периодических изданиях › Обзорная статья › Рецензирование
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TY - JOUR
T1 - Scattered Radiation of Protoplanetary Disks
AU - Grinin, Vladimir P.
AU - Tambovtseva, Larisa V.
PY - 2022/4/1
Y1 - 2022/4/1
N2 - Scattered radiation of circumstellar (CS) dust plays an important role in the physics of young stars. Its observational manifestations are various but more often they are connected with the appearance of intrinsic polarization in young stars and their CS disks. In our brief review we consider two classes of astrophysical objects in which the participation of scattered radiation is key for understanding their nature. First of all, these are irregular variables (UX Ori type stars). The modern idea of their nature and the mechanism of their variability has been formed thanks to synchronous observations of their linear polarization and brightness. The second class of objects is the CS disks themselves. Their detailed investigation became possible due to observations in polarized light using a coronographic technique and large telescopes.
AB - Scattered radiation of circumstellar (CS) dust plays an important role in the physics of young stars. Its observational manifestations are various but more often they are connected with the appearance of intrinsic polarization in young stars and their CS disks. In our brief review we consider two classes of astrophysical objects in which the participation of scattered radiation is key for understanding their nature. First of all, these are irregular variables (UX Ori type stars). The modern idea of their nature and the mechanism of their variability has been formed thanks to synchronous observations of their linear polarization and brightness. The second class of objects is the CS disks themselves. Their detailed investigation became possible due to observations in polarized light using a coronographic technique and large telescopes.
KW - linear polarization
KW - protoplanetary disk
KW - RW Aur
KW - scattered radiation
KW - UX Ori stars
UR - http://www.scopus.com/inward/record.url?scp=85128356713&partnerID=8YFLogxK
U2 - 10.3390/universe8040224
DO - 10.3390/universe8040224
M3 - Review article
AN - SCOPUS:85128356713
VL - 8
JO - Universe
JF - Universe
SN - 2218-1997
IS - 4
M1 - 224
ER -
ID: 126125409