Many types of variable stars obey strict relationships between their pulsation periods and brightnesses. The contributions in this volume offer significant new insights from a wealth of recent observations into the periodâ luminosity relations governing pulsating variables and their implications for the cosmic distance scale.
Many types of variable stars obey strict relationships between their pulsation periods and brightnesses. The contributions in this volume offer significant new insights from a wealth of recent observations into the periodâ luminosity relations governing pulsating variables and their implications for the cosmic distance scale.Hinweis: Dieser Artikel kann nur an eine deutsche Lieferadresse ausgeliefert werden.
Produktdetails
Produktdetails
Proceedings of the International Astronomical Union Symposia and Colloquia
Part I. Setting the Scene - The Extragalactic 'Problem': The Cepheid extragalactic distance scale: Past, present and future Wendy Freedman; The local value of H0 Adam Riess; The tip of the Red Giant Branch as a cosmological probe Myung Gyoon Lee; Period-luminosity relations in the Local Group of galaxies Igor Soszy ski; Part II. Stellar Pulsation Physics: Theoretical stellar pulsation physics Marcella Marconi; Anomalous Cepheids: Updated theoretical period-luminosity-color and period-wesenheit relations Giulia De Somma; Pulsation of chemically peculiar stars Ernst Paunzen; A study of the stellar photosphere-hydrogen ionization front interaction in Scuti stars Mami Deka; A multi-wavelength analysis of BL Her stars: Models vs observations Susmita Das; Part III. Primary Period-Luminosity Relation Calibrators in the Milky Way: Cepheids and RR Lyrae Gisella Clementini; Primary PL-relation calibrators in the Milky Way: Cepheids and RR Lyrae: Physical basis, calibration, and applications Martin Groenewegen; Cepheids with giant companions: A new, abundant source of Cepheid astrophysics Bogumi Pilecki; Part IV. Disentangling the Structural Components of the Milky Way: Implication of the period-magnitude relation for massive AGB stars and its astronomical applications Akiharu Nakagawa; The structure of the Milky Way from period-luminosity relations Dorota Skowron; Granulation in red supergiants: The scaling relations Yi Ren; The distance scale of Type II Cepheids from near infrared observations in the Magellanic Clouds Teresa Sicignano; Binary star masses and distances from interferometry Alexandre Gallenne; Globular clusters metallicity and distance from their RR Lyrae stars light curves Armando Arellano Ferro; The PL diagram for Sct stars: back in business as distance estimators Antonio García Hernández; Part V. Period-Luminosity Relations in the Nearby Universe: Period-Luminosity-Metallicity relations for classical pulsators at near-infrared wavelengths Anupam Bhardwaj; A multiphase study of classical Cepheids in the Magellanic Clouds - Models and observations Kerdaris Kurbah; Double-mode RR Lyrae star - robust distance and metallicity indicators Shu Wang; Empirical constraints for the instability strip from the analysis of LMC Cepheids Felipe Espinoza-Arancibia; Part VI. Non-traditional Period-Luminosity Relations: The period-luminosity relations of red supergiants Biwei Jiang; Long-period variables as distance and age indicators in the era of Gaia and LSST Michele Trabucchi; China Space Station Telescope and variable star studies Xiaodian Chen; OH/IR stars and the period-luminosity relation of Mira variables Dieter Engels.
Part I. Setting the Scene - The Extragalactic 'Problem': The Cepheid extragalactic distance scale: Past, present and future Wendy Freedman; The local value of H0 Adam Riess; The tip of the Red Giant Branch as a cosmological probe Myung Gyoon Lee; Period-luminosity relations in the Local Group of galaxies Igor Soszy ski; Part II. Stellar Pulsation Physics: Theoretical stellar pulsation physics Marcella Marconi; Anomalous Cepheids: Updated theoretical period-luminosity-color and period-wesenheit relations Giulia De Somma; Pulsation of chemically peculiar stars Ernst Paunzen; A study of the stellar photosphere-hydrogen ionization front interaction in Scuti stars Mami Deka; A multi-wavelength analysis of BL Her stars: Models vs observations Susmita Das; Part III. Primary Period-Luminosity Relation Calibrators in the Milky Way: Cepheids and RR Lyrae Gisella Clementini; Primary PL-relation calibrators in the Milky Way: Cepheids and RR Lyrae: Physical basis, calibration, and applications Martin Groenewegen; Cepheids with giant companions: A new, abundant source of Cepheid astrophysics Bogumi Pilecki; Part IV. Disentangling the Structural Components of the Milky Way: Implication of the period-magnitude relation for massive AGB stars and its astronomical applications Akiharu Nakagawa; The structure of the Milky Way from period-luminosity relations Dorota Skowron; Granulation in red supergiants: The scaling relations Yi Ren; The distance scale of Type II Cepheids from near infrared observations in the Magellanic Clouds Teresa Sicignano; Binary star masses and distances from interferometry Alexandre Gallenne; Globular clusters metallicity and distance from their RR Lyrae stars light curves Armando Arellano Ferro; The PL diagram for Sct stars: back in business as distance estimators Antonio García Hernández; Part V. Period-Luminosity Relations in the Nearby Universe: Period-Luminosity-Metallicity relations for classical pulsators at near-infrared wavelengths Anupam Bhardwaj; A multiphase study of classical Cepheids in the Magellanic Clouds - Models and observations Kerdaris Kurbah; Double-mode RR Lyrae star - robust distance and metallicity indicators Shu Wang; Empirical constraints for the instability strip from the analysis of LMC Cepheids Felipe Espinoza-Arancibia; Part VI. Non-traditional Period-Luminosity Relations: The period-luminosity relations of red supergiants Biwei Jiang; Long-period variables as distance and age indicators in the era of Gaia and LSST Michele Trabucchi; China Space Station Telescope and variable star studies Xiaodian Chen; OH/IR stars and the period-luminosity relation of Mira variables Dieter Engels.
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