High Resolution Infrared Spectroscopy (37 results)

Hardcover. Condition: Sehr gut. XX, 559 S. : Ill. Very good. Shrink wrapped. Sprache: Englisch Gewicht in Gramm: 1125.

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Condition: Used. pp. 584.

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Hardcover. Condition: 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.…

Condition: Used. pp. 584.

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Buch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - 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. …

Taschenbuch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - 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.…

Condition: New. pp. xx + 599 Softcover reprint of hardcover 1st ed. 2005 edition.

Condition: New. In English.

Gr.-8°, OKart. 1. ed. XX, 559 p. Shelfmark on spine, stamp on title and preliminary page, otherwise fine copy. Sprache: Englisch Gewicht in Gramm: 0.

Paperback. Condition: Brand New. 579 pages. 9.00x6.00x1.31 inches. In Stock.

Taschenbuch. Condition: Neu. High Resolution Infrared Spectroscopy in Astronomy | Proceedings of an ESO Workshop Held at Garching, Germany, 18-21 November 2003 | Hans Ulrich Käufl (u. a.) | Taschenbuch | ESO Astrophysics Symposia | xx | Englisch | 2010 | Springer | EAN 9783642064401 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu.…

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Taschenbuch. Condition: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -The infrared spectral region between wavelengths of 2 and 6 µm is of great importance in molecular physics. Molecules with an X-H bond (X being carbon, nitrogen or oxygen) exhibit strong vibrational transitions there, but also linear carbon clusters Cn (n=2,3,¿). Many combination bands and overtones of low-energy vibrational modes also occur in this spectral range. Analyses of these spectral features allow ¿ if highly resolved ¿ for example the prediction of pure rotational transitions in the sub-mm wavelength regime, or help understanding the internal dynamics of the molecule.To provide radiation sources with extremely large frequency coverage, two optical parametric oscillator (OPO) systems in the wavelength regions from 2.5 to 4.1 µm and from 4.7 to 5.4 µm have been set up and characterized in this thesis. The OPO system around 5 µm wavelength is the only one in this spectral region used in high-resolution spectroscopy up to now. Both of the OPO systems have been shown to be ideal tools for spectroscopic studies delivering highly accurate transition frequencies of transient molecules, using the following example cases: The rovibrational spectrum of the fundamental cation CH2D+ around 3.2 µm wavelength has been measured with unprecedented spectral resolution and frequency accuracy. The combination of the OPO as radiation source with a cold ion trap to produce and store the ions has been proven to have a high predictive power for pure rotational transition frequencies of CH2D+. Located at around 100 to 200 GHz, these are of great importance in astrophysics. The V3 fundamental vibration of Si2C3 around 5.1 µm wavelength has been measured using the OPO and a newly built jet spectrometer for the production of transient molecules. Molecular parameters have been determined with high precision. An associated hot band originating from the V7 vibrational bending mode has been resolved and analyzed for the first time. The pure carbon clusters C3 and C7 have also been examined. For the first time, a combination band of C3 and an associated hot band were detected around 3.0 µm wavelength in the gas phase. Their analyses yield valuable information about the potential energy surface of C3. Analysis of the V5 mode of C7 delivered further proof of its rigidity, which was put into question by earlier works. Last but not least, a previously unknown associated hot band of C7 has been detected and analyzed. 162 pp. Englisch.…

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Leather Bound. Condition: New. Language: English. Language: English. Presenting an Exquisite Leather-Bound Edition, expertly crafted with Original Natural Leather that gracefully adorns the spine and corners. The allure continues with Golden Leaf Printing that adds a touch of elegance, while Hand Embossing on the rounded spine lends an artistic flair. This masterpiece has been meticulously reprinted in 2025, utilizing the invaluable guidance of the original edition published many years ago in 1988. The contents of this book are presented in classic black and white. Its durability is ensured through a meticulous sewing binding technique, enhancing its longevity. Imprinted on top-tier quality paper. A team of professionals has expertly processed each page, delicately preserving its content without alteration. Due to the vintage nature of these books, every page has been manually restored for legibility. However, in certain instances, occasional blurriness, missing segments, or faint black spots might persist. We sincerely hope for your understanding of the challenges we faced with these books. Recognizing their significance for readers seeking insight into our historical treasure, we've diligently restored and reissued them. Our intention is to offer this valuable resource once again. We eagerly await your feedback, hoping that you'll find it appealing and will generously share your thoughts and recommendations. Lang: - English, Pages:- 72, Print on Demand. If it is a multi-volume set, then it is only a single volume. We are specialised in Customisation of books, if you wish to opt different color leather binding, you may contact us. This service is chargeable. Product Disclaimer: Kindly be informed that, owing to the inherent nature of leather as a natural material, minor discolorations or textural variations may be perceptible. Explore the FOLIO EDITION (12x19 Inches): Available Upon Request. 72 72.…

Buch. Condition: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -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. 559 pp. Englisch.…

Taschenbuch. Condition: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -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. 580 pp. Englisch.…

Taschenbuch. Condition: Neu. This item is printed on demand - Print on Demand Titel. Neuware -The infrared spectral region between wavelengths of 2 and 6 µm is of great importance in molecular physics. Molecules with an X-H bond (X being carbon, nitrogen or oxygen) exhibit strong vibrational transitions there, but also linear carbon clusters Cn (n=2,3.). Many combination bands and overtones of low-energy vibrational modes also occur in this spectral range. Analyses of these spectral features allow - if highly resolved - for example the prediction of pure rotational transitions in the sub-mm wavelength regime, or help understanding the internal dynamics of the molecule.To provide radiation sources with extremely large frequency coverage, two optical parametric oscillator (OPO) systems in the wavelength regions from 2.5 to 4.1 µm and from 4.7 to 5.4 µm have been set up and characterized in this thesis. The OPO system around 5 µm wavelength is the only one in this spectral region used in high-resolution spectroscopy up to now. Both of the OPO systems have been shown to be ideal tools for spectroscopic studies delivering highly accurate transition frequencies of transient molecules, using the following example cases:The rovibrational spectrum of the fundamental cation CH2D+ around 3.2 µm wavelength has been measured with unprecedented spectral resolution and frequency accuracy. The combination of the OPO as radiation source with a cold ion trap to produce and store the ions has been proven to have a high predictive power for pure rotational transition frequencies of CH2D+. Located at around 100 to 200 GHz, these are of great importance in astrophysics.The V3 fundamental vibration of Si2C3 around 5.1 µm wavelength has been measured using the OPO and a newly built jet spectrometer for the production of transient molecules. Molecular parameters have been determined with high precision. An associated hot band originating from the V7 vibrational bending mode has been resolved and analyzed for the first time.The pure carbon clusters C3 and C7 have also been examined. For the first time, a combination band of C3 and an associated hot band were detected around 3.0 µm wavelength in the gas phase. Their analyses yield valuable information about the potential energy surface of C3. Analysis of the V5 mode of C7 delivered further proof of its rigidity, which was put into question by earlier works. Last but not least, a previously unknown associated hot band of C7 has been detected and analyzed.Cuvillier Verlag, Nonnenstieg 8, 37075 Göttingen 162 pp. Englisch.…