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Variable and Non-spherical Stellar Winds in Luminous Hot Stars (Record no. 12355)

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000 -LEADER
fixed length control field	06381nam a22004935i 4500
001 - CONTROL NUMBER
control field	978-3-540-49062-3
003 - CONTROL NUMBER IDENTIFIER
control field	DE-He213
005 - DATE AND TIME OF LATEST TRANSACTION
control field	20190213151926.0
007 - PHYSICAL DESCRIPTION FIXED FIELD--GENERAL INFORMATION
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020 ## - INTERNATIONAL STANDARD BOOK NUMBER
International Standard Book Number	9783540490623
--	978-3-540-49062-3
024 7# - OTHER STANDARD IDENTIFIER
Standard number or code	10.1007/BFb0106346
Source of number or code	doi
050 #4 - LIBRARY OF CONGRESS CALL NUMBER
Classification number	QB4
072 #7 - SUBJECT CATEGORY CODE
Subject category code	PG
Source	bicssc
072 #7 - SUBJECT CATEGORY CODE
Subject category code	SCI004000
Source	bisacsh
072 #7 - SUBJECT CATEGORY CODE
Subject category code	PG
Source	thema
082 04 - DEWEY DECIMAL CLASSIFICATION NUMBER
Classification number	520
Edition number	23
245 10 - TITLE STATEMENT
Title	Variable and Non-spherical Stellar Winds in Luminous Hot Stars
Medium	[electronic resource] :
Remainder of title	Proceedings of the IAU Colloquium No. 169 Held in Heidelberg, Germany, 15–19 June 1998 /
Statement of responsibility, etc	edited by Bernhard Wolf, Otmar Stahl, Alex W. Fullerton.
264 #1 -
--	Berlin, Heidelberg :
--	Springer Berlin Heidelberg,
--	1999.
300 ## - PHYSICAL DESCRIPTION
Extent	XX, 428 p. 171 illus.
Other physical details	online resource.
336 ## -
--	text
--	txt
--	rdacontent
337 ## -
--	computer
--	c
--	rdamedia
338 ## -
--	online resource
--	cr
--	rdacarrier
347 ## -
--	text file
--	PDF
--	rda
490 1# - SERIES STATEMENT
Series statement	Lecture Notes in Physics,
International Standard Serial Number	0075-8450 ;
Volume number/sequential designation	523
505 0# - FORMATTED CONTENTS NOTE
Formatted contents note	Rotationally modulated winds of O stars -- Rotationally modulated winds of BA-type supergiants -- Using spectropolarimetry to determine envelope geometry and test variability models for hot star circumstellar envelopes -- Disks of classical be stars -- Evidence for azimuthal asymmetry in be star winds -- Short and medium term variability of emission lines in selected southern Be stars -- Disk winds of B[e] supergiants -- Polarimetric evidence of non-spherical winds -- Wolf-rayet wind models: Photometric and polarimetric variability -- Anisotropic outflows from LBVs and Ofpe/WN9 stars -- Non-isotropic outflows in the infrared: ISO imaging of LBVs -- Radio evidence for non-isotropic outflows from hot stars -- Optical interferometry of non-spherical winds -- Direct observational evidence for magnetic fields in hot stars -- HST WFPCII observations of the inner HR car nebula -- Observing hot stars in all four stokes parameters -- Inverse spectropolarimetric modelling of hot star wind structure and variability -- Physics of radiatively driven winds by high angular resolution observations (HARO) -- Wind-compressed disks -- Non-spherical radiation-driven wind models -- Radiation-driven disk winds -- Radiative fluxes and forces in non-spherical winds -- Line-driven ablation by external irradiation -- Extremely luminous atmospheres -- Disks formed by rotation induced bi-stability -- The effects of magnetic fields on the winds from luminous hot stars -- Modeling oblique rotators: Magnetospheres and winds -- X-ray emission from magnetically confined winds -- O-star wind variability in the ultraviolet and optical range -- X-ray evidence for wind instabilities -- X-ray variability of the O star ? Puppis -- On the variable winds of BA supergiants -- UV wind variability in B supergiants and its implications for wind structures -- Variability and evidence of non-spherical stellar winds in A-type supergiants -- Variable winds in early-B hypergiants -- Wind variations of wolf-rayet stars -- Spectral analyses of wolf-rayet stars: The impact of clumping -- The long-term variability of luminous blue variables -- Blitz model for the eruptions of eta carinae -- Short-term variations of LBV’s -- Imaging polarimetry of eta carinae with the hubble space telescope -- Non-spherical outflows in massive binary systems: Circumbinary disks? -- Long-term behaviour of the variable wind of P Cygni -- High-resolution spectroscopy of stellar winds in recently recognized LBV candidates -- Evidence for wind anisotropies from dust formation by wolf-rayet stars -- ISO-SWS spectroscopy of B[e] stars -- The line-driven instability -- Co-rotating interaction regions in 2D hot-star wind models with line-driven instability -- Pulsations in O stars -- Non-radial pulsations of BA supergiants and Be stars -- Theory of pulsational instabilities of hot stars -- Non-radially pulsating hot stars: Non-radial pulsations and Be phenomenon -- Pulsation hydrodynamics of luminous blue variables and pulsation-driven winds -- Linear strange modes in massive stars -- Instabilities in LBVs and WR stars -- The evolution of non-spherical and non-stationary winds of massive stars -- Rotation and anisotropic losses of mass and angular momentum -- Rotation and wolf-rayet star formation -- Dusty LBV nebulae: Tracing the mass loss history of the most massive stars -- Wolf-rayet and LBV nebulae as the result of variable and non-spherical stellar winds -- Ring nebulae abundances: Probes of the evolutionary history of luminous blue variable stars -- The wind momentum — Luminosity relationship of blue supergiants -- Conference summary: The demise of spherical and stationary winds.
520 ## - SUMMARY, ETC.
Summary, etc	There is abundant evidence that essentially all luminous hot-star winds contain time-dependent and anisotropic structures. IAU Colloquium 169 was convened to review the observations of variability and asphericity, to discuss the physical processes that might cause such behavior and to look for evolutionary consequences. The topics included OBA stars, Be stars, Wolf-Rayet stars, Be stars, and luminous blue variables (LBVs). The role played by rotation in shaping the stellar wind was a recurrent theme. Photospheric pulsations and/or magnetic fields are particularly appealing mechanisms for triggering the formation of recurrent wind structures.
650 14 - SUBJECT ADDED ENTRY--TOPICAL TERM
Topical term or geographic name as entry element	Astronomy, Observations and Techniques.
--	http://scigraph.springernature.com/things/product-market-codes/P22014
650 24 - SUBJECT ADDED ENTRY--TOPICAL TERM
Topical term or geographic name as entry element	Astrophysics and Astroparticles.
--	http://scigraph.springernature.com/things/product-market-codes/P22022
700 1# - ADDED ENTRY--PERSONAL NAME
Personal name	Wolf, Bernhard.
Relator term	editor.
Relator code	edt
--	http://id.loc.gov/vocabulary/relators/edt
700 1# - ADDED ENTRY--PERSONAL NAME
Personal name	Stahl, Otmar.
Relator term	editor.
Relator code	edt
--	http://id.loc.gov/vocabulary/relators/edt
700 1# - ADDED ENTRY--PERSONAL NAME
Personal name	Fullerton, Alex W.
Relator term	editor.
Relator code	edt
--	http://id.loc.gov/vocabulary/relators/edt
710 2# - ADDED ENTRY--CORPORATE NAME
Corporate name or jurisdiction name as entry element	SpringerLink (Online service)
773 0# - HOST ITEM ENTRY
Title	Springer eBooks
776 08 - ADDITIONAL PHYSICAL FORM ENTRY
Display text	Printed edition:
International Standard Book Number	9783662142103
776 08 - ADDITIONAL PHYSICAL FORM ENTRY
Display text	Printed edition:
International Standard Book Number	9783662142097
776 08 - ADDITIONAL PHYSICAL FORM ENTRY
Display text	Printed edition:
International Standard Book Number	9783540657026
830 #0 - SERIES ADDED ENTRY--UNIFORM TITLE
Uniform title	Lecture Notes in Physics,
--	0075-8450 ;
Volume number/sequential designation	523
856 40 - ELECTRONIC LOCATION AND ACCESS
Uniform Resource Identifier	https://doi.org/10.1007/BFb0106346
912 ## -
--	ZDB-2-PHA
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--	ZDB-2-LNP
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--	ZDB-2-BAE

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