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

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書目名稱High Resolution Infrared Spectroscopy in Astronomy影響因子(影響力)




書目名稱High Resolution Infrared Spectroscopy in Astronomy影響因子(影響力)學(xué)科排名




書目名稱High Resolution Infrared Spectroscopy in Astronomy網(wǎng)絡(luò)公開(kāi)度




書目名稱High Resolution Infrared Spectroscopy in Astronomy網(wǎng)絡(luò)公開(kāi)度學(xué)科排名




書目名稱High Resolution Infrared Spectroscopy in Astronomy被引頻次




書目名稱High Resolution Infrared Spectroscopy in Astronomy被引頻次學(xué)科排名




書目名稱High Resolution Infrared Spectroscopy in Astronomy年度引用




書目名稱High Resolution Infrared Spectroscopy in Astronomy年度引用學(xué)科排名




書目名稱High Resolution Infrared Spectroscopy in Astronomy讀者反饋




書目名稱High Resolution Infrared Spectroscopy in Astronomy讀者反饋學(xué)科排名

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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

OPINE

Culmination

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.

頭腦冷靜

FLAG

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.

配置

intimate

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.

Basilar-Artery

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.

BALK