High Resolution Infrared Spectroscipy in Astronomy: Proceedings of an Eso Workshop Held at Garchig, Germany, 18-21 November 2003 - Rilegato
Sinossi
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 HII-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 synthetic spectra and reports on laboratory spectra. In this sense, a fruitful exchange between molecular physics and astronomy was again accomplished and is documented in this volume.
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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 HII-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 synthetic spectra and reports on laboratory spectra. In this sense, a fruitful exchange between molecular physics and astronomy was again accomplished and is documented in this volume.
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High resolution infrared spectroscopy in astronomy : proceedings of an ESO workshop held at Garching, Germany, 18 - 21 November 2003. ESO Astrophysics Symposia.
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High Resolution Infrared Spectroscopy In Astronomy: Proceedings Of An Eso Workshop Held At Garching, Germany, 18-21 November 2003 (eso Astrophysics Symposia
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High Resolution Infrared Spectroscipy in Astronomy : Proceedings of an Eso Workshop Held at Garchig, Germany, 18-21 November 2003
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High Resolution Infrared Spectroscopy in Astronomy: Proceedings of an ESO Workshop Held at Garching, Germany, 18-21 November 2003 (ESO Astrophysics Symposia)
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Hardcover. Condizione: Near Fine. Hardcover, xx + 559 pages, NOT ex-library. Printed in Germany. Book is clean and bright throughout with unmarked text, free of inscriptions and stamps, firmly bound. Minor external handling wear. Issued without a dust jacket. -- Incomplete Contents: 1 Instrumentation & Observational Highlights: - High-Resolution Frontier in Infrared Spectroscopy; CRIRES: Context & Status; Science Highlights from 4 Years of NIRSPEC on the Keck II Telescope; Extragalactic Science at Very High Spectral Resolution; High-Resolution Spectroscopy with Michelle on UKIRT; High-Resolution Mid-Infrared Molecular Spectroscopy of Star Forming Regions with TEXES; PEPSI, the High-Resolution Optical-IR Spectrograph for the LBT; Atomic Data in the 1-5 [mu]m Region: Present Status; High-Resolution Spectroscopy on the Milliarcsecond Scale; Don't Waste a Single Photon: Power of Deconvolution in High-Resolution Spectroscopy; R=100,000 Spectroscopy of Photodissociation Regions : H2 Rotational Lines in the Orion Bar; T-ReCS and Michelle: Mid-infrared Spectroscopic Capabilities of the Gemini Observatory; Improving the Accuracy of HCN/hNC Opacity Data & Accounting for Isotopomers; SIFTIR: Spectro-Polarimetric Imaging Fourier Transform Spectrometer for the Infrared; Mid-infrared Spectroscopic Standards; GIANO: Ultra-stable IR Echelle Spectrometer for the TNG Telescope; Correcting the Chromatic & Airmass Dependent Extinction for TIMMI2 Spectra; Active Galaxies in the Mid-infrared Ground-based vs Space-born Observations; 2 Young Stars, Hot Stars, LBVs, Novae, SNe, ISM-1: - Infrared Spectroscopy of H+3 in the Interstellar Medium; Identifying Molecular Outflow Drivers Using High-resolution NIR Spectroscopy; Tests for the Magnetospheric Accretion Model for Young Low Mass Stars; Probing T Tauri Stars & Their Circumstellar Environment at NIR High Spectral Resolution; Near-IR Spectroscopy of Deeply Embedded, Young Massive Stars; A VLT/ISAAC Study of Massive YSOs in UCHII Regions; Carbon Isotope Ratio in Local Molecular Clouds; R=100,000 Mid-IR Spectroscopy of UCHII Regions: High Resolution is Worth It; VLT-ISAAC 3-5 [mu]m Spectroscopy of Low-mass Young Stellar Objects: Prospects for CRIRERS; Probing the Embedded YSOs of the R CrA Region Through VLT-ISAAC Spectroscopy; Outflows in Regions of Star Formation; H2 Mid-IR Emission from Young Stars: TEXES/IRTF Survey; High-resolution Infrared Spectroscopy of Protoplanetary Disks; Linear Spectropolarimetry of Young & Other Emission Line Stars; Interpreting the Hydrogen IR Lines: Impact of Improved Electron Collision Data; Third Body in the Eclipsing Binaries AR Aurigae & TX Herculis; Small- to Large-scale Properties of Protostellar Jets Through High-resolution IR Spectroscopy; TIMMI2 & VLT-ISAAC Spectroscopy of Circumstellar Dust Disks: Spatially Resolved 3.3 [mu]m PAH Feature Around HD 100546; Absorption Line Survey of H+3 Towards the Galactic Center; Molecular Hydrogen Absorption Line Detected in Dense Molecular Clouds; Detection of Reactive Ions Towards UC HII Regions; Active Stars & He I 10830 A: EUV Connection; Molecular Chemistry in Gaseous Disks Around Young Hot Stars; 4.7 [mu]m CO & H2 Line Emission in NGC 2071; 3 Normal MS Stars, Old Stars, Active Stars, ISM-2: - Dynamic Model Atmospheres of Cool Giants; Synthetic Line Profiles for Pulsating Red Giants; IR Spectroscopy of AGB Stars; Molecules as Probe of the Temperature Distribution in the Atmosphere of Cool Giants; Infrared Spectra of Red Giants: Molecular & Atomic Lines; Tracing Accretion onto Herbig Ae/Be Stars Using Near-infrared Spectroscopy; Magnetic Fields & Stellar Surface Structures; Infrared Observations of Magnetic Fields on Young Stars; Magnetic Fields & Atmospheric Motions in Pulsating Stars; Post-AGB Objects & Planetary Nebulae; Chemical Abundances in the Galactic Bulge; COmospheres & Beyond; Abundance of Elements in Cool Stars; 4 Solar Systems, Brown Dwarfs; 5 Our Solar System. Codice articolo 005876
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High Resolution Infrared Spectroscopy in Astronomy
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