Probing the Chemistry of Molecular Cores: 2.5-5 μm AKARI Grism Spectroscopy of Young Stellar Objects in B35A

被引：0

作者：

Noble, Jennifer A. ^{[1
]}

Aikawa, Yuri

Fraser, Helen J. ^{[1
]}

Pontoppidan, Klaus M.

Sakon, Itsuki

机构：

[1] Univ Strathclyde, Scottish Univ Phys Alliance, Dept Phys, John Anderson Bldg,107 Rottenrow, Glasgow G4 0NG, Lanark, Scotland

来源：

AKARI, A LIGHT TO ILLUMINATE THE MISTY UNIVERSE | 2009年 / 418卷

关键词：

STAR-FORMATION; ICES; EVOLUTION; CLOUDS; H2O; CO2;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

2.5-5 mu m spectra of four embedded protostars in the molecular core B35A were extracted using a novel data reduction pipeline developed for AKARI near infrared (NIR) grism spectroscopy. Column densities of the solid phase species present in the four lines of sight were calculated, illustrating the sensitivity of AKARI. The importance of ice spectra of low luminosity protostars to the development of star formation theories is discussed.

引用

页码：411 / +

页数：2

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