The Origin of Outflows in Evolved Stars (Iau S366)
Herausgeber: Decin, Leen; Gielen, Clio; Zijlstra, Albert
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The Origin of Outflows in Evolved Stars (Iau S366)
Herausgeber: Decin, Leen; Gielen, Clio; Zijlstra, Albert
- Gebundenes Buch
All stars are known to power strong stellar winds at the end of their lives, expelling stellar material that is recycled as building blocks of new planets and life. IAU S366 provides an overview of state-of-the-art observational, theoretical and numerical studies on the origin of winds in evolved stars.
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All stars are known to power strong stellar winds at the end of their lives, expelling stellar material that is recycled as building blocks of new planets and life. IAU S366 provides an overview of state-of-the-art observational, theoretical and numerical studies on the origin of winds in evolved stars.
Produktdetails
- Produktdetails
- Proceedings of the International Astronomical Union Symposia and Colloquia
- Verlag: Cambridge University Press
- Seitenzahl: 400
- Erscheinungstermin: 2. März 2023
- Englisch
- Abmessung: 238mm x 166mm x 6mm
- Gewicht: 724g
- ISBN-13: 9781108490795
- ISBN-10: 1108490794
- Artikelnr.: 65341195
- Proceedings of the International Astronomical Union Symposia and Colloquia
- Verlag: Cambridge University Press
- Seitenzahl: 400
- Erscheinungstermin: 2. März 2023
- Englisch
- Abmessung: 238mm x 166mm x 6mm
- Gewicht: 724g
- ISBN-13: 9781108490795
- ISBN-10: 1108490794
- Artikelnr.: 65341195
Preface; Getting started: how a supersonic stellar wind is initiated from a
hydrostatic surface; The first 3D models of evolved hot star outflows; The
origin and impact of Wolf-Rayet-type mass loss; Magnetised gas nebulae of
evolved massive stars; Can pre-supernova winds from massive stars enrich
the interstellar medium with nitrogen at high redshift?; Effects of wind
mass-loss on the observational properties of type Ib and Ic supernova
progenitors; Environments of evolved massive stars: evidence for episodic
mass ejections; How did the stellar winds of massive stars influence the
surrounding environment in the Galactic Center?; The role of mass loss in
chemodynamical evolution of galaxies; The interplay between mass-loss and
binarity; The link between hot and cool outflows; Atmospheric structure and
dynamics of evolved massive stars thanks to 3D radiative hydrodynamical
simulations of stellar convection; The Great Dimming of Betelgeuse from the
VLT/VLTI; The inner dust shell of Betelgeuse seen with polarimetry;
Analytic, turbulent pressure driven mass loss rates from red supergiants;
Multiple shell ejections on a 100 yr timescale from a massive yellow
hypergiant; BOSS-3D: a binary object spectral synthesis code in 3D;
Simulations of colliding winds in massive binary systems with accretion;
Mass loss from binary stars approaching merger; Explaining the winds of AGB
stars: Recent progress; The onset of mass loss in evolved stars; The
distribution of carbonaceous molecules and SiN around the S-type AGB star W
Aquilae; Long-term light curve variations of AGB stars: episodic mass-loss
or binarity?; MATISSE first pictures of dust and molecules around R
Sculptoris; Tracing the role of AGB stars in the Galactic fluorine budget;
Tracing the inner regions of circumstellar envelopes via high-excitation
water transitions; Detailing evolved star wind complexity: comparing maser
and thermal imaging; Mass-loss rates of cool evolved stars in M33 galaxy;
Shaping the initial-final mass relation of white dwarfs with AGB outflows;
Mass transfer in AGB binaries: uncovering a new evolution channel by 3D
radiation-hydrodynamic simulations; Route towards complete 3D
hydro-chemical simulations of companion-perturbed AGB outflows; 3D
hydrodynamical survey of the impact of a companion on the morphology and
dynamics of AGB outflows; Morpho-kinematics around cool evolved stars
unveiling the underlying companion; Accretion-powered Outflows in AGB
Stars; Learning about AGB stars by studying the stars polluted by their
outflows; Tc-rich M stars: platypuses of low-mass star evolution; The
impact of UV photons from a stellar companion on the chemistry of AGB
outflows; Chemistry on hot astrochemical dust surfaces: sulfur in AGB
outflows; Circumbinary discs around post-AGB binaries as a result of binary
interactions: an infrared interferometric view; Pre-planetary nebulae: A
context for principles, progress, and questions on how binaries and
magnetic fields produce jets; ALMA (finally!) discloses a rotating
disk+bipolar wind system at the centre of the wind-prominent pPN
OH231.8+4.2; Lessons from the ionised and molecular mass of post-CE PNe;
Outflows and disks in post-RGB objects: products of common envelope
ejection?; RGB mass loss: inferences from CMD-fitting and asteroseismology;
Towards the identification of carriers of the unidentified infrared (UIR)
bands in novae; Author index.
hydrostatic surface; The first 3D models of evolved hot star outflows; The
origin and impact of Wolf-Rayet-type mass loss; Magnetised gas nebulae of
evolved massive stars; Can pre-supernova winds from massive stars enrich
the interstellar medium with nitrogen at high redshift?; Effects of wind
mass-loss on the observational properties of type Ib and Ic supernova
progenitors; Environments of evolved massive stars: evidence for episodic
mass ejections; How did the stellar winds of massive stars influence the
surrounding environment in the Galactic Center?; The role of mass loss in
chemodynamical evolution of galaxies; The interplay between mass-loss and
binarity; The link between hot and cool outflows; Atmospheric structure and
dynamics of evolved massive stars thanks to 3D radiative hydrodynamical
simulations of stellar convection; The Great Dimming of Betelgeuse from the
VLT/VLTI; The inner dust shell of Betelgeuse seen with polarimetry;
Analytic, turbulent pressure driven mass loss rates from red supergiants;
Multiple shell ejections on a 100 yr timescale from a massive yellow
hypergiant; BOSS-3D: a binary object spectral synthesis code in 3D;
Simulations of colliding winds in massive binary systems with accretion;
Mass loss from binary stars approaching merger; Explaining the winds of AGB
stars: Recent progress; The onset of mass loss in evolved stars; The
distribution of carbonaceous molecules and SiN around the S-type AGB star W
Aquilae; Long-term light curve variations of AGB stars: episodic mass-loss
or binarity?; MATISSE first pictures of dust and molecules around R
Sculptoris; Tracing the role of AGB stars in the Galactic fluorine budget;
Tracing the inner regions of circumstellar envelopes via high-excitation
water transitions; Detailing evolved star wind complexity: comparing maser
and thermal imaging; Mass-loss rates of cool evolved stars in M33 galaxy;
Shaping the initial-final mass relation of white dwarfs with AGB outflows;
Mass transfer in AGB binaries: uncovering a new evolution channel by 3D
radiation-hydrodynamic simulations; Route towards complete 3D
hydro-chemical simulations of companion-perturbed AGB outflows; 3D
hydrodynamical survey of the impact of a companion on the morphology and
dynamics of AGB outflows; Morpho-kinematics around cool evolved stars
unveiling the underlying companion; Accretion-powered Outflows in AGB
Stars; Learning about AGB stars by studying the stars polluted by their
outflows; Tc-rich M stars: platypuses of low-mass star evolution; The
impact of UV photons from a stellar companion on the chemistry of AGB
outflows; Chemistry on hot astrochemical dust surfaces: sulfur in AGB
outflows; Circumbinary discs around post-AGB binaries as a result of binary
interactions: an infrared interferometric view; Pre-planetary nebulae: A
context for principles, progress, and questions on how binaries and
magnetic fields produce jets; ALMA (finally!) discloses a rotating
disk+bipolar wind system at the centre of the wind-prominent pPN
OH231.8+4.2; Lessons from the ionised and molecular mass of post-CE PNe;
Outflows and disks in post-RGB objects: products of common envelope
ejection?; RGB mass loss: inferences from CMD-fitting and asteroseismology;
Towards the identification of carriers of the unidentified infrared (UIR)
bands in novae; Author index.
Preface; Getting started: how a supersonic stellar wind is initiated from a
hydrostatic surface; The first 3D models of evolved hot star outflows; The
origin and impact of Wolf-Rayet-type mass loss; Magnetised gas nebulae of
evolved massive stars; Can pre-supernova winds from massive stars enrich
the interstellar medium with nitrogen at high redshift?; Effects of wind
mass-loss on the observational properties of type Ib and Ic supernova
progenitors; Environments of evolved massive stars: evidence for episodic
mass ejections; How did the stellar winds of massive stars influence the
surrounding environment in the Galactic Center?; The role of mass loss in
chemodynamical evolution of galaxies; The interplay between mass-loss and
binarity; The link between hot and cool outflows; Atmospheric structure and
dynamics of evolved massive stars thanks to 3D radiative hydrodynamical
simulations of stellar convection; The Great Dimming of Betelgeuse from the
VLT/VLTI; The inner dust shell of Betelgeuse seen with polarimetry;
Analytic, turbulent pressure driven mass loss rates from red supergiants;
Multiple shell ejections on a 100 yr timescale from a massive yellow
hypergiant; BOSS-3D: a binary object spectral synthesis code in 3D;
Simulations of colliding winds in massive binary systems with accretion;
Mass loss from binary stars approaching merger; Explaining the winds of AGB
stars: Recent progress; The onset of mass loss in evolved stars; The
distribution of carbonaceous molecules and SiN around the S-type AGB star W
Aquilae; Long-term light curve variations of AGB stars: episodic mass-loss
or binarity?; MATISSE first pictures of dust and molecules around R
Sculptoris; Tracing the role of AGB stars in the Galactic fluorine budget;
Tracing the inner regions of circumstellar envelopes via high-excitation
water transitions; Detailing evolved star wind complexity: comparing maser
and thermal imaging; Mass-loss rates of cool evolved stars in M33 galaxy;
Shaping the initial-final mass relation of white dwarfs with AGB outflows;
Mass transfer in AGB binaries: uncovering a new evolution channel by 3D
radiation-hydrodynamic simulations; Route towards complete 3D
hydro-chemical simulations of companion-perturbed AGB outflows; 3D
hydrodynamical survey of the impact of a companion on the morphology and
dynamics of AGB outflows; Morpho-kinematics around cool evolved stars
unveiling the underlying companion; Accretion-powered Outflows in AGB
Stars; Learning about AGB stars by studying the stars polluted by their
outflows; Tc-rich M stars: platypuses of low-mass star evolution; The
impact of UV photons from a stellar companion on the chemistry of AGB
outflows; Chemistry on hot astrochemical dust surfaces: sulfur in AGB
outflows; Circumbinary discs around post-AGB binaries as a result of binary
interactions: an infrared interferometric view; Pre-planetary nebulae: A
context for principles, progress, and questions on how binaries and
magnetic fields produce jets; ALMA (finally!) discloses a rotating
disk+bipolar wind system at the centre of the wind-prominent pPN
OH231.8+4.2; Lessons from the ionised and molecular mass of post-CE PNe;
Outflows and disks in post-RGB objects: products of common envelope
ejection?; RGB mass loss: inferences from CMD-fitting and asteroseismology;
Towards the identification of carriers of the unidentified infrared (UIR)
bands in novae; Author index.
hydrostatic surface; The first 3D models of evolved hot star outflows; The
origin and impact of Wolf-Rayet-type mass loss; Magnetised gas nebulae of
evolved massive stars; Can pre-supernova winds from massive stars enrich
the interstellar medium with nitrogen at high redshift?; Effects of wind
mass-loss on the observational properties of type Ib and Ic supernova
progenitors; Environments of evolved massive stars: evidence for episodic
mass ejections; How did the stellar winds of massive stars influence the
surrounding environment in the Galactic Center?; The role of mass loss in
chemodynamical evolution of galaxies; The interplay between mass-loss and
binarity; The link between hot and cool outflows; Atmospheric structure and
dynamics of evolved massive stars thanks to 3D radiative hydrodynamical
simulations of stellar convection; The Great Dimming of Betelgeuse from the
VLT/VLTI; The inner dust shell of Betelgeuse seen with polarimetry;
Analytic, turbulent pressure driven mass loss rates from red supergiants;
Multiple shell ejections on a 100 yr timescale from a massive yellow
hypergiant; BOSS-3D: a binary object spectral synthesis code in 3D;
Simulations of colliding winds in massive binary systems with accretion;
Mass loss from binary stars approaching merger; Explaining the winds of AGB
stars: Recent progress; The onset of mass loss in evolved stars; The
distribution of carbonaceous molecules and SiN around the S-type AGB star W
Aquilae; Long-term light curve variations of AGB stars: episodic mass-loss
or binarity?; MATISSE first pictures of dust and molecules around R
Sculptoris; Tracing the role of AGB stars in the Galactic fluorine budget;
Tracing the inner regions of circumstellar envelopes via high-excitation
water transitions; Detailing evolved star wind complexity: comparing maser
and thermal imaging; Mass-loss rates of cool evolved stars in M33 galaxy;
Shaping the initial-final mass relation of white dwarfs with AGB outflows;
Mass transfer in AGB binaries: uncovering a new evolution channel by 3D
radiation-hydrodynamic simulations; Route towards complete 3D
hydro-chemical simulations of companion-perturbed AGB outflows; 3D
hydrodynamical survey of the impact of a companion on the morphology and
dynamics of AGB outflows; Morpho-kinematics around cool evolved stars
unveiling the underlying companion; Accretion-powered Outflows in AGB
Stars; Learning about AGB stars by studying the stars polluted by their
outflows; Tc-rich M stars: platypuses of low-mass star evolution; The
impact of UV photons from a stellar companion on the chemistry of AGB
outflows; Chemistry on hot astrochemical dust surfaces: sulfur in AGB
outflows; Circumbinary discs around post-AGB binaries as a result of binary
interactions: an infrared interferometric view; Pre-planetary nebulae: A
context for principles, progress, and questions on how binaries and
magnetic fields produce jets; ALMA (finally!) discloses a rotating
disk+bipolar wind system at the centre of the wind-prominent pPN
OH231.8+4.2; Lessons from the ionised and molecular mass of post-CE PNe;
Outflows and disks in post-RGB objects: products of common envelope
ejection?; RGB mass loss: inferences from CMD-fitting and asteroseismology;
Towards the identification of carriers of the unidentified infrared (UIR)
bands in novae; Author index.