COLD DUST AROUND CHAMELEON STARS

被引：7

作者：

HENNING, T

THAMM, E

机构：

[1] Max Planck Society, Research group 'Dust in Star-forming Regions', Jena

来源：

ASTROPHYSICS AND SPACE SCIENCE | 1994年 / 212卷 / 1-2期

关键词：

D O I：

10.1007/BF00984525

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Here we present the results of 1.3 millimetre continuum measurements for intermediate-mass stars in the Chamaeleon system of dark clouds. The detected millimetre radiation is most probably thermal emission from cold circumstellar dust grains. The measured millimetre fluxes are combined with infrared observations to model the broad-band spectral energy distribution (SED). In this way the parameters of the emission regions are determined.

引用

页码：215 / 220

页数：6

共 23 条

[1]

ASSENDORP R, 1990, MON NOT R ASTRON SOC, V247, P624

[2] A SURVEY FOR CIRCUMSTELLAR DISKS AROUND YOUNG STELLAR OBJECTS [J].