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2015 Fiscal Year Final Research Report

Observational Study of planet formation by exploring edge of gap and arm on protoplanetary disks

Research Project

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Project/Area Number 25800107
Research Category

Grant-in-Aid for Young Scientists (B)

Allocation TypeMulti-year Fund
Research Field Astronomy
Research InstitutionThe Graduate University for Advanced Studies

Principal Investigator

MAYAMA SATOSHI  総合研究大学院大学, 学内共同利用施設等, 講師 (20553267)

Project Period (FY) 2013-04-01 – 2016-03-31
Keywords赤外線天文学
Outline of Final Research Achievements

Most stars form as multiples. Although the planet formation around a single star has been well proceeded, that around multiples remains many unexplained mysteries. Therefore, high resolution imaging observations of binary disks are conducted in order to gain better understanding of planet formation around multiples.
As one of the unique result, polarization imaging data of binary disks with non-axisymmetric features have been obtained. By comparisons with radio data including ALMA, origin of the non-axisymmetric features are analyzed.

Free Research Field

数物系科学

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Published: 2017-05-10   Modified: 2018-03-22  

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