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Indirect evidence of significant grain growth in young protostellar envelopes from polarized dust emission

机译：来自极化粉尘排放的年轻抗原群信封显着的谷物生长的间接证据

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Valeska Valdivia; Anaëlle Maury; Robert Brauer; Patrick Hennebelle; Maud Galametz; Vincent Guillet; Stefan Reissl;
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1. SILICATE EMISSION PROFILES FROM LOW-MASS PROTOSTELLAR DISKS IN THE ORION NEBULA: EVIDENCE FOR GROWTH AND THERMAL PROCESSING OF GRAINS [J] . R. Y. Shuping, Marc Kassis, Mark Morris, The Astrophysical journal . 2006,第1Pt2期

机译：猎户座星云中低质量原恒生硅的硅酸盐排放特征：晶粒长大和热处理的证据
2. SILICATE EMISSION PROFILES FROM LOW-MASS PROTOSTELLAR DISKS IN THE ORION NEBULA: EVIDENCE FOR GROWTH AND THERMAL PROCESSING OF GRAINS [J] . R. Y. Shuping, Marc Kassis, Mark Morris, The Astrophysical journal . 2006,第1Pt2期

机译：猎户座星云中低质量原恒生硅的硅酸盐排放特征：谷物生长和热处理的证据
3. SILICATE EMISSION PROFILES FROM LOW-MASS PROTOSTELLAR DISKS IN THE ORION NEBULA: EVIDENCE FOR GROWTH AND THERMAL PROCESSING OF GRAINS [J] . R. Y. Shuping, Marc Kassis, Mark Morris, The Astrophysical journal . 2006,第1Pt2期

机译：猎户座星云中低质量原恒生硅的硅酸盐排放特征：谷物生长和热处理的证据
4. PILOT: a balloon-borne experiment to measure the polarized FIR emission of dust grains in the interstellar medium [C] . R. Misawa, J-Ph. Bernard, P. Ade, Conference on millimeter, submillimeter, and far-infrared detectors and instrumentation for astronomy . 2014

机译：PILOT：气球飞行实验，用于测量星际介质中尘埃粒子的极化FIR发射
5. Dust grain growth and disk evolution of a set of young stellar objects. [D] . Carpenter, William Joseph. 2008

机译：一组年轻的恒星物体的尘埃颗粒生长和盘状演化。
6. The Abundance of SiC2 in Carbon Star Envelopes: Evidence that SiC2 is a gas-phase precursor of SiC dust [O] . Sarah Massalkhi, M. Agúndez, J. Cernicharo, -1

机译：碳星信封中SiC2的丰度：证明SiC2是SiC粉尘的气相前驱体
7. Silicate Emission Profiles from Low-Mass Protostellar Disks in the Orion Nebula: Evidence for Growth and Thermal Processing of Grains [O] . Shuping R Y, Kassis M, Morris M, 2006

机译：猎户星云中低质量原恒星盘的硅酸盐排放特征：谷物生长和热处理的证据
8. Dust Coagulation in Infalling Protostellar Envelopes I. Compact Grains [R] . Yorke, H., Suttner, G., Lin, D. 1999

机译：打击原始星形信封中的粉尘凝固I.紧凑型谷物

Indirect evidence of significant grain growth in young protostellar envelopes from polarized dust emission

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