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Age-dating a star-burst with GEMINI/CIRPASS observations of the core of M83
被引:4
|作者:
Sharp, RG
Parry, IR
Ryder, SD
Knapen, JH
Mazzuca, LM
机构:
[1] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England
[2] Anglo Australian Observ, Epping, NSW 1710, Australia
[3] Univ Hertfordshire, Hatfield AL10 9AB, Herts, England
[4] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
关键词:
galaxies : starburst;
galaxies : stellar content;
instrumentation : spectrographs;
D O I:
10.1002/asna.200310186
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
We present Preliminary results from a set of near-IR integral field spectroscopic observations of the central, star-burst, regions of the barred spiral galaxy M83, obtained with CIR-PASS on Gemini-S. We present maps in the Pabeta and [FeII] 1.257 mum emission lines which appear surprisingly different. We outline the procedure in which we will use Pabetaemission line strengths and measures of CO absorption to determine the relative and absolute ages of individual star-forming knots in the central kpc region of M83.
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页码:108 / 111
页数:4
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