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Physics of Luminous Blue Variables

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Cover of 'Physics of Luminous Blue Variables'

Table of Contents

  1. Altmetric Badge
    Book Overview
  2. Altmetric Badge
    Chapter 1 Physics of Luminous Blue Variables
  3. Altmetric Badge
    Chapter 2 On the Evolutionary Status and Instability Mechanism of the Luminous Blue Variables (LBV)
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    Chapter 3 Evolutionary Diagnostics of LBV Spectra and Systems in the LMC
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    Chapter 4 The Distribution of Types of Liminous Blue Variables
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    Chapter 5 Age of Luminous Blue Variable Candidates from their Stellar and Nebular Environment
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    Chapter 6 An Ultraviolet View of the Luminous Blue Variables
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    Chapter 7 Photometric Variability of Luminous Blue Variables in Quiescent State
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    Chapter 8 Model Atmospheres and Quantitative Spectroscopy of Luminous Blue Stars
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    Chapter 9 The H-R Diagrams of The LMC and SMC
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    Chapter 10 Physics of Luminous Blue Variables
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    Chapter 11 Plinian Eruptions Á La Eta Carinae
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    Chapter 12 Changes in the Atmospheric Structure of LBV’s During Eruptions
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    Chapter 13 The B[e] Stars
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    Chapter 14 Modeling Mass Loss from B[e] Stars
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    Chapter 15 Luminous Blue Variables Need Not Be Blue
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    Chapter 16 Mass Ejections from the G-Type Hypergiant HR 8752
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    Chapter 17 Mass Loss from Luminous Blue Variables
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    Chapter 18 Circumstellar Ejecta Around LBV’s
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    Chapter 19 High Resolution Coronographic Imaging of AG Carinae
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    Chapter 20 Infrared Observations of Circumstellar Ejecta Around Luminous Blue Variables
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    Chapter 21 The Formation of Shells in the Wind from P Cygni
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    Chapter 22 Close Binary Models for Luminous Blue Variable Stars
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    Chapter 23 The Role of Radiation Pressure in LBV Atmospheres
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    Chapter 24 The Role of Rotation in Luminous Blue Variables
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    Chapter 25 Atmospheric Dynamics of Luminous Stars
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    Chapter 26 Theoretical Relations Between LBVs and Other Stars
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    Chapter 27 Observational Connections Between LBV’S and Other Stars, With Emphasis On Wolf-Rayet Stars
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    Chapter 28 First Panel Discussion
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    Chapter 29 Second Panel Discussion
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    Chapter 30 P Cygni: The Star that Started it All
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    Chapter 31 The Wind of P Cygni
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    Chapter 32 A Source for Mass-Low Instabilities in LBV’s — The Case of P Cygni
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    Chapter 33 The Ionization and Thermal Balance in P Cygni’s Wind revisited
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    Chapter 34 Variable Flux of P Cygni in Continuum and Spectral Lines
  36. Altmetric Badge
    Chapter 35 Optical and UV Investigation of the Envelope of AG Carinae
  37. Altmetric Badge
    Chapter 36 AG Car: Variability, Extinction, Distance and Luminosity
  38. Altmetric Badge
    Chapter 37 The optical micro variations of the two S Dor type stars AG Car and HR Car
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    Chapter 38 On the Periodicity of Hubble-Sandage Objects in M 31
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    Chapter 39 ETA Carinae: UV Constraints on Possible Models
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    Chapter 40 High Resolution Emission Line Profiles in Blue Luminous Stars
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    Chapter 41 Analysis of LBV Circumstellar Envelopes Using FeII Lines
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    Chapter 42 On the Interpretation of Emission Wings of Balmer Lines in LBV’S
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    Chapter 43 Atmospheric Models for LBV’s at Minimum and Maximum States
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    Chapter 44 Atmospheric Parameters and Accelerations in the Outer Parts of Luminous Hot Stars
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    Chapter 45 NLTE Analysis of R84
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    Chapter 46 Physics of Instabilities in Radiatively Driven Stellar Winds
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    Chapter 47 Far Infrared Circumstellar “Debris” Shells: Clues to the Evolution of Massive Stars?
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    Chapter 48 High-Dispersion Spectroscopy of the B[e] Supergiants S 111
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    Chapter 49 Slash Stars: Two Types, Two Scenarios?
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    Chapter 50 Blobs in the Winds of Wolf-Rayet Stars
  52. Altmetric Badge
    Chapter 51 LSS4005 and NaSt1, Two Galactic Ofpe/WN or B[e] Objects
Overall attention for this book and its chapters
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About this Attention Score

  • Above-average Attention Score compared to outputs of the same age (60th percentile)
  • Good Attention Score compared to outputs of the same age and source (77th percentile)

Mentioned by

wikipedia
1 Wikipedia page

Citations

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30 Dimensions

Readers on

mendeley
2 Mendeley
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Title
Physics of Luminous Blue Variables
Published by
ADS, December 2012
DOI 10.1007/978-94-009-1031-7
ISBNs
978-9-40-106955-7, 978-9-40-091031-7
Editors

Davidson, Kris, Moffat, A. F. J., Lamers, H. J. G. L. M.

Mendeley readers

The data shown below were compiled from readership statistics for 2 Mendeley readers of this research output. Click here to see the associated Mendeley record.

Geographical breakdown

Country Count As %
Unknown 2 100%

Demographic breakdown

Readers by professional status Count As %
Student > Ph. D. Student 1 50%
Student > Bachelor 1 50%
Readers by discipline Count As %
Physics and Astronomy 2 100%

Attention Score in Context

This research output has an Altmetric Attention Score of 3. This is our high-level measure of the quality and quantity of online attention that it has received. This Attention Score, as well as the ranking and number of research outputs shown below, was calculated when the research output was last mentioned on 26 May 2016.
All research outputs
#4,013,735
of 13,462,296 outputs
Outputs from ADS
#6,276
of 26,212 outputs
Outputs of similar age
#102,667
of 271,059 outputs
Outputs of similar age from ADS
#34
of 189 outputs
Altmetric has tracked 13,462,296 research outputs across all sources so far. This one is in the 49th percentile – i.e., 49% of other outputs scored the same or lower than it.
So far Altmetric has tracked 26,212 research outputs from this source. They receive a mean Attention Score of 4.2. This one is in the 33rd percentile – i.e., 33% of its peers scored the same or lower than it.
Older research outputs will score higher simply because they've had more time to accumulate mentions. To account for age we can compare this Altmetric Attention Score to the 271,059 tracked outputs that were published within six weeks on either side of this one in any source. This one has gotten more attention than average, scoring higher than 60% of its contemporaries.
We're also able to compare this research output to 189 others from the same source and published within six weeks on either side of this one. This one has done well, scoring higher than 77% of its contemporaries.