Evolution of Southern Star-Forming Regions

被引:0
|
作者
P. Ehrenfreund
E.F. Van Dishoeck
M. Burgdorf
J. Cami
P. Van Hoof
A.G.G.M. Tielens
W.A. Schutte
W.F. Thi
机构
[1] Leiden Observatory,
[2] ISO Science Operation Center,undefined
[3] ESA/VILSPA,undefined
[4] SRON Groningen,undefined
[5] Kapteyn Astronomical Institute,undefined
关键词
Hydrocarbon; PAHs; Aromatic Hydrocarbon; Short Wavelength; Emission Line;
D O I
10.1023/A:1001162818288
中图分类号
学科分类号
摘要
We present ISO observations of bright, high-mass southern starforming regions with the Short Wavelength Spectrometer (SWS) and Long Wavelength Spectrometer (LWS). The selected targets show a range of pre-main sequence evolutionary phases. Whereas some objects still show interstellar ice features, the most evolved objects are coincident with ultra-compact HII regions and show strong emission lines from atomic species and polycyclic aromatic hydrocarbons (PAHs). We discuss the ISO spectra between 2.5 - 200 µm of selected southern star-forming regions in the context of their evolution.
引用
收藏
页码:83 / 89
页数:6
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