The snowline in the protoplanetary disk and extrasolar plane

发布时间：2018-06-18 01:47

本文选题：snowline—planets + and　；参考：《Research in Astronomy and Astrophysics》2017年08期

【摘要】：We investigate the behavior of the snowline in a protoplanetary disk and the relationship between the radius of the snowline and properties of molecular cloud cores.In our disk model,we consider mass influx from the gravitational collapse of a molecular cloud core,irradiation from the central star,and thermal radiation from the ambient molecular cloud gas.As the protoplanetary disk evolves,the radius of the snowline increases first to a maximum value Rmax,and then decreases in the late stage of evolution of the protoplanetary disk.The value of Rmaxis dependent on the properties of molecular cloud cores(mass M_(core),angular velocity ω and temperature T_(core)).Many previous works found that solid material tends to accumulate at the location of the snowline,which suggests that the snowline is the preferred location for giant planet formation.With these conclusions,we compare the values of R_(max) with semimajor axes of giant planets in extrasolar systems,and find that Rmaxmay provide an upper limit for the locations of the formation of giant planets which are formed by the core accretion model.
[Abstract]:We investigate the behavior of the snowline in a protoplanetary disk and the relationship between the radius of the snowline and properties of molecular cloud cores.In our disk model,we consider mass influx from the gravitational collapse of a molecular cloud core,irradiation from the central star,and thermal radiation from the ambient molecular cloud gas.As the protoplanetary disk evolves,the radius of the snowline increases first to a maximum value Rmax,and then decreases In the late stage of evolution of the protoplanetary disk.the value of Rmaxis dependent on the properties of molecular cloud cores(mass dependent on the properties of molecular cloud cores(mass velocity omega and temperature previous works found that solid material tends to accumulate at the location of the snowline which suggests that the snowline is the preferred location for giant planet formation.With these conclusionswe compare the values of Rad max.) with semimajor axes of giant planets in extrasolar systems sans and Find that Rmaxmay provide an upper limit for the locations of the formation of giant planets which are formed by the core accretion model.
【作者单位】： College
【基金】：supported by the National Natural Science Foundation of China (Grant No. 11504150)
【分类号】：P15

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