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Titlebook: High Resolution Infrared Spectroscopy in Astronomy; Proceedings of an ES Hans Ulrich Käufl,Ralf Siebenmorgen,Alan F. M. Moo Conference proc

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发表于 2025-3-21 17:51:44 | 显示全部楼层 |阅读模式
书目名称High Resolution Infrared Spectroscopy in Astronomy
副标题Proceedings of an ES
编辑Hans Ulrich Käufl,Ralf Siebenmorgen,Alan F. M. Moo
视频video
概述Includes supplementary material:
丛书名称ESO Astrophysics Symposia
图书封面Titlebook: High Resolution Infrared Spectroscopy in Astronomy; Proceedings of an ES Hans Ulrich Käufl,Ralf Siebenmorgen,Alan F. M. Moo Conference proc
描述.Two specialized new instruments for ESO‘s VLT, VISIR and CRIRES, spawned the idea for this workshop. CRIRES is a dedicated very high resolution infrared spectrograph; VISIR features a high resolution spectroscopic mode. Together, the instruments combine the sensitivity of an 8m-telescope with the now well-established reliability of VLT-facility instruments. High resolution here means that lines in cool stellar atmospheres and H.II.-regions can be resolved. The astrophysical topics discussed in this rather specialized workshop range from the inner solar system to active galactic nuclei. There are many possibilities for new discoveries with these instruments, but the unique capability, which becomes available through high-resolution infrared spectroscopy, is the observation of molecular rotational-vibrational transitions in many astrophysical environments. Particularly interesting and surprising in this context, many papers on modeling and laboratory spectroscopy at the workshop appear to indicate that astronomical observations are lagging a bit behind in this field. The papers are an interesting mix of reports from existing high resolution facilities, reports on modeling efforts of
出版日期Conference proceedings 2005
关键词Active Galaxies; Astronomical Observation; High Resolution Infrared Spectroscopy; Interstellar Medium; P
版次1
doihttps://doi.org/10.1007/b96749
isbn_softcover978-3-642-06440-1
isbn_ebook978-3-540-31606-0Series ISSN 1431-2433 Series E-ISSN 1611-6143
issn_series 1431-2433
copyrightSpringer-Verlag Berlin Heidelberg 2005
The information of publication is updating

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发表于 2025-3-21 22:06:58 | 显示全部楼层
Conference proceedings 2005red spectrograph; VISIR features a high resolution spectroscopic mode. Together, the instruments combine the sensitivity of an 8m-telescope with the now well-established reliability of VLT-facility instruments. High resolution here means that lines in cool stellar atmospheres and H.II.-regions can b
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发表于 2025-3-22 07:03:06 | 显示全部楼层
Mid Infrared Spectroscopic Standards: Observations and Models,9). This allows us to demonstrate that the derived absolute calibration of the spectra is accurate to better than 5% in most cases. Our subsample of MIR calibration standards presented here shall become the primary calibrators of the VISIR instrument.
发表于 2025-3-22 11:07:36 | 显示全部楼层
发表于 2025-3-22 13:23:37 | 显示全部楼层
Active Galaxies in the Mid Infrared: Ground-Based versus Space-Born Observations, emission is only detected in starbursts whereas PAH features are significantly reduced or completely absent in AGN. We find that the mid-infrared emission of Seyferts is dominated by a compact core while the starbursts are spatially resolved.
发表于 2025-3-22 18:51:49 | 显示全部楼层
发表于 2025-3-22 22:53:56 | 显示全部楼层
CRIRES: Context and Status,in the near infrared. This aspect in fact motivated the organization of this workshop to both explore the scientific prospects and prepare the ESO community for the use of the instrument in the not too distant future. Here I will summarize the main characteristics of the instrument and its development status.
发表于 2025-3-23 02:17:31 | 显示全部楼层
Improving the Accuracy of HCN/HNC Opacity Data and Accounting for Isotopomers,r ab initio counterparts. Thus improving the accuracy of many of the strongest HCN/HNC line frequencies. We propose to generate an approximate H.CN linelist using experimentally determined energy levels of H.CN with our HCN line intensities. Our preliminary results are presented here.
发表于 2025-3-23 07:22:59 | 显示全部楼层
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