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Luminosity calibration of low redshift quasars / / E. Joseph Wampler, principal investigator
| Luminosity calibration of low redshift quasars / / E. Joseph Wampler, principal investigator |
| Autore | Wampler E. Joseph |
| Pubbl/distr/stampa | Santa Cruz, California : , : University of California |
| Descrizione fisica | 1 online resource (3 unnumbered pages) |
| Collana | NASA-CR |
| Soggetto topico |
Quasars
Stellar luminosity IUE Long wave radiation Radio galaxies Red shift |
| Formato | Materiale a stampa  |
| Livello bibliografico | Monografia |
| Lingua di pubblicazione | eng |
| Record Nr. | UNINA-9910702536503321 |
Wampler E. Joseph
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| Santa Cruz, California : , : University of California | ||
| Materiale a stampa | ||
| Lo trovi qui: Univ. Federico II | ||
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A panchromatic view of galaxies [[electronic resource] /] / Alessandro Boselli
| A panchromatic view of galaxies [[electronic resource] /] / Alessandro Boselli |
| Autore | Boselli Alessandro <1965-> |
| Pubbl/distr/stampa | Weinheim, : Wiley-VCH Verlag, c2012 |
| Descrizione fisica | 1 online resource (342 p.) |
| Disciplina | 523.112 |
| Soggetto topico |
Galaxies
Radio astronomy Radio galaxies |
| Soggetto genere / forma | Electronic books. |
| ISBN |
1-283-86982-9
3-527-64027-4 3-527-64025-8 3-527-64026-6 |
| Formato | Materiale a stampa |
| Livello bibliografico | Monografia |
| Lingua di pubblicazione | eng |
| Nota di contenuto |
A Panchromatic View of Galaxies; Contents; Preface; 1 Introduction; 1.1 Galaxies; 1.2 A Multifrequency Approach; 1.3 The Purpose of this Book; Part One Emitting Sources and Radiative Processes in Galaxies; 2 X-ray; 2.1 Continuum; 2.1.1 Discrete Sources; 2.1.2 X-ray Emission in Active Galaxies; 2.1.3 Hot Gas; 3 UV-Optical-NIR; 3.1 Continuum: Stellar Emission; 3.2 Emission Lines; 3.2.1 Hydrogen Lines; 3.2.2 Metals; 3.3 Absorption Lines; 3.3.1 Hydrogen Lines; 3.3.2 Other Elements; 3.4 Molecular Lines; 3.4.1 H2 Near-Infrared Emission Lines; 3.4.2 H2 UV Absorption Lines; 4 The Infrared
4.1 Continuum: Dust Emission4.2 Emission Lines; 4.2.1 PAHs; 4.2.2 Cooling Lines in PDR; 4.2.3 H2 Lines; 4.2.4 Dust Absorption of Ly Scattered Photons; 5 Millimeter and Centimeter Radio; 5.1 Continuum; 5.1.1 Free-Free Emission; 5.1.2 Synchrotron Emission; 5.1.3 Dust Emission; 5.2 Emission Lines; 5.2.1 Molecular Lines; 5.2.2 HI; 5.3 Absorption Lines; 5.3.1 HI; Part Two Derived Quantities; 6 Properties of the Hot X-ray Emitting Gas; 6.1 X-ray Luminosity; 6.2 Gas Temperature; 7 Dust Properties; 7.1 The Far-IR Luminosity; 7.2 Dust Mass and Temperature; 8 Radio Properties 8.1 Determining the Contribution of the Different Radio Components8.1.1 Synchrotron vs. Free--Free Radio Emission in the Centimeter Domain; 8.1.2 The Emission of the Cold Dust Component at 1.5 mm; 8.2 The Radio Luminosity; 9 The Spectral Energy Distribution; 9.1 The Emission in the UV to Near-Infrared Spectral Domain; 9.1.1 UV, Optical, and Near-IR Colors; 9.1.2 Fitting SEDs with Population Synthesis Models; 9.2 The Dust Emission in the Infrared Domain; 9.2.1 Mid- and Far-Infrared Colors; 9.3 The Thermal and Nonthermal Radio Emission; 10 Spectral Features 10.1 Galaxy Characterization through Emission and Absorption Lines10.1.1 Classification of the Nuclear Activity; 10.1.2 Classification of Post-Starburst and Post-Star-Forming Galaxies; 10.1.3 Line Diagnostics; 10.2 Gas Metallicity from Emission Lines; 10.3 Stellar Age and Metallicity from Absorption Lines; 11 Gas Properties; 11.1 Gas Density, Mass, and Temperature; 11.1.1 The Atomic HI Mass; 11.1.2 The Molecular H2 Mass; 12 Dust Extinction; 12.1 Galactic Extinction; 12.1.1 Extinction Curve; 12.2 Internal Attenuation; 12.2.1 Attenuation of the Emission Lines 12.2.2 Attenuation of the Stellar Continuum13 Star Formation Tracers; 13.1 The Initial Mass Function; 13.2 The Star Formation Rate; 13.3 The Birthrate Parameter and the Specific Star Formation Rate; 13.4 The Star Formation Efficiency and the Gas Consumption Time Scale; 13.5 Hydrogen Emission Lines; 13.6 UV Stellar Continuum; 13.7 Infrared; 13.7.1 Integrated Infrared Luminosity; 13.7.2 Monochromatic Infrared Luminosities; 13.8 Radio Continuum; 13.9 Other Indicators; 13.9.1 The X-ray Luminosity; 13.9.2 Forbidden Lines; 13.9.3 [CII]; 13.9.4 Radio Recombination Lines 13.10 Population Synthesis Models |
| Record Nr. | UNINA-9910141337203321 |
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Boselli Alessandro <1965->
|
||
| Weinheim, : Wiley-VCH Verlag, c2012 | ||
| Materiale a stampa | ||
| Lo trovi qui: Univ. Federico II | ||
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A panchromatic view of galaxies / / Alessandro Boselli
| A panchromatic view of galaxies / / Alessandro Boselli |
| Autore | Boselli Alessandro <1965-> |
| Pubbl/distr/stampa | Weinheim, : Wiley-VCH Verlag, c2012 |
| Descrizione fisica | 1 online resource (342 p.) |
| Disciplina | 523.112 |
| Soggetto topico |
Galaxies
Radio astronomy Radio galaxies |
| ISBN |
9781283869829
1283869829 9783527640270 3527640274 9783527640256 3527640258 9783527640263 3527640266 |
| Formato | Materiale a stampa |
| Livello bibliografico | Monografia |
| Lingua di pubblicazione | eng |
| Nota di contenuto |
A Panchromatic View of Galaxies; Contents; Preface; 1 Introduction; 1.1 Galaxies; 1.2 A Multifrequency Approach; 1.3 The Purpose of this Book; Part One Emitting Sources and Radiative Processes in Galaxies; 2 X-ray; 2.1 Continuum; 2.1.1 Discrete Sources; 2.1.2 X-ray Emission in Active Galaxies; 2.1.3 Hot Gas; 3 UV-Optical-NIR; 3.1 Continuum: Stellar Emission; 3.2 Emission Lines; 3.2.1 Hydrogen Lines; 3.2.2 Metals; 3.3 Absorption Lines; 3.3.1 Hydrogen Lines; 3.3.2 Other Elements; 3.4 Molecular Lines; 3.4.1 H2 Near-Infrared Emission Lines; 3.4.2 H2 UV Absorption Lines; 4 The Infrared
4.1 Continuum: Dust Emission4.2 Emission Lines; 4.2.1 PAHs; 4.2.2 Cooling Lines in PDR; 4.2.3 H2 Lines; 4.2.4 Dust Absorption of Ly Scattered Photons; 5 Millimeter and Centimeter Radio; 5.1 Continuum; 5.1.1 Free-Free Emission; 5.1.2 Synchrotron Emission; 5.1.3 Dust Emission; 5.2 Emission Lines; 5.2.1 Molecular Lines; 5.2.2 HI; 5.3 Absorption Lines; 5.3.1 HI; Part Two Derived Quantities; 6 Properties of the Hot X-ray Emitting Gas; 6.1 X-ray Luminosity; 6.2 Gas Temperature; 7 Dust Properties; 7.1 The Far-IR Luminosity; 7.2 Dust Mass and Temperature; 8 Radio Properties 8.1 Determining the Contribution of the Different Radio Components8.1.1 Synchrotron vs. Free--Free Radio Emission in the Centimeter Domain; 8.1.2 The Emission of the Cold Dust Component at 1.5 mm; 8.2 The Radio Luminosity; 9 The Spectral Energy Distribution; 9.1 The Emission in the UV to Near-Infrared Spectral Domain; 9.1.1 UV, Optical, and Near-IR Colors; 9.1.2 Fitting SEDs with Population Synthesis Models; 9.2 The Dust Emission in the Infrared Domain; 9.2.1 Mid- and Far-Infrared Colors; 9.3 The Thermal and Nonthermal Radio Emission; 10 Spectral Features 10.1 Galaxy Characterization through Emission and Absorption Lines10.1.1 Classification of the Nuclear Activity; 10.1.2 Classification of Post-Starburst and Post-Star-Forming Galaxies; 10.1.3 Line Diagnostics; 10.2 Gas Metallicity from Emission Lines; 10.3 Stellar Age and Metallicity from Absorption Lines; 11 Gas Properties; 11.1 Gas Density, Mass, and Temperature; 11.1.1 The Atomic HI Mass; 11.1.2 The Molecular H2 Mass; 12 Dust Extinction; 12.1 Galactic Extinction; 12.1.1 Extinction Curve; 12.2 Internal Attenuation; 12.2.1 Attenuation of the Emission Lines 12.2.2 Attenuation of the Stellar Continuum13 Star Formation Tracers; 13.1 The Initial Mass Function; 13.2 The Star Formation Rate; 13.3 The Birthrate Parameter and the Specific Star Formation Rate; 13.4 The Star Formation Efficiency and the Gas Consumption Time Scale; 13.5 Hydrogen Emission Lines; 13.6 UV Stellar Continuum; 13.7 Infrared; 13.7.1 Integrated Infrared Luminosity; 13.7.2 Monochromatic Infrared Luminosities; 13.8 Radio Continuum; 13.9 Other Indicators; 13.9.1 The X-ray Luminosity; 13.9.2 Forbidden Lines; 13.9.3 [CII]; 13.9.4 Radio Recombination Lines 13.10 Population Synthesis Models |
| Record Nr. | UNINA-9911018937403321 |
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Boselli Alessandro <1965->
|
||
| Weinheim, : Wiley-VCH Verlag, c2012 | ||
| Materiale a stampa | ||
| Lo trovi qui: Univ. Federico II | ||
| ||
Soggetto topico
-
Radio galaxies
(3)
- Galaxies (2)
- Radio astronomy (2)
- IUE (1)
- Long wave radiation (1)