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Physics, Formation and Evolution of Rotating Stars

Overview of attention for book
Cover of 'Physics, Formation and Evolution of Rotating Stars'

Table of Contents

  1. Altmetric Badge
    Book Overview
  2. Altmetric Badge
    Chapter 1 The Mechanical Equilibrium of Stars
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    Chapter 2 The Mechanical Equilibrium of Rotating Stars
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    Chapter 3 The Energetic Equilibrium of Stars
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    Chapter 4 The Energy Conservation and Radiative Equilibrium in Rotating Stars
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    Chapter 5 Stellar Convection
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    Chapter 6 Overshoot, Semiconvection, Thermohaline Convection, Rotation and Solberg–Hoiland Criterion
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    Chapter 7 The Equation of State
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    Chapter 8 The Opacities
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    Chapter 9 Nuclear Reactions and Neutrino Processes
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    Chapter 10 Transport Processes: Diffusion and Advection
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    Chapter 11 Meridional Circulation
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    Chapter 12 Rotation-Driven Instabilities
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    Chapter 13 Magnetic Field Instabilities and Transport Processes
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    Chapter 14 Physics of Mass Loss by Stellar Winds
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    Chapter 15 Radial Pulsations of Stars
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    Chapter 16 Nonradial Stellar Oscillations
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    Chapter 17 Transport by Gravity Waves
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    Chapter 18 Pre-stellar Phase
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    Chapter 19 The Protostellar Phase and Accretion Disks
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    Chapter 20 The Pre-main Sequence Phase and the Birthlines
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    Chapter 21 Rotation in Star Formation
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    Chapter 22 The Formation of Massive Stars
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    Chapter 23 The Formation of First Stars in the Universe: Pop. III and Pop. II.5 Stars
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    Chapter 24 Solutions of the Equations and Simple Models
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    Chapter 25 Evolution in the H-Burning Phases
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    Chapter 26 Evolution in the He Burning and AGB Phases of Low and Intermediate Mass Stars with Rotation
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    Chapter 27 Massive Star Evolution with Mass Loss and Rotation
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    Chapter 28 Advanced Evolutionary Stages and Pre-supernovae
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    Chapter 29 Evolution of Z = 0 and Very Low Z Stars
Overall attention for this book and its chapters
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About this Attention Score

  • Good Attention Score compared to outputs of the same age (71st percentile)
  • Good Attention Score compared to outputs of the same age and source (67th percentile)

Mentioned by

twitter
1 X user
wikipedia
17 Wikipedia pages

Citations

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480 Dimensions

Readers on

mendeley
72 Mendeley
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Title
Physics, Formation and Evolution of Rotating Stars
Published by
ADS, December 2008
DOI 10.1007/978-3-540-76949-1
ISBNs
978-3-54-076948-4, 978-3-54-076949-1
Authors

Maeder, André

X Demographics

X Demographics

The data shown below were collected from the profile of 1 X user who shared this research output. Click here to find out more about how the information was compiled.
Mendeley readers

Mendeley readers

The data shown below were compiled from readership statistics for 72 Mendeley readers of this research output. Click here to see the associated Mendeley record.

Geographical breakdown

Country Count As %
Brazil 3 4%
Germany 2 3%
Canada 1 1%
Chile 1 1%
Unknown 65 90%

Demographic breakdown

Readers by professional status Count As %
Student > Ph. D. Student 24 33%
Student > Master 13 18%
Researcher 11 15%
Student > Bachelor 5 7%
Student > Postgraduate 4 6%
Other 11 15%
Unknown 4 6%
Readers by discipline Count As %
Physics and Astronomy 64 89%
Environmental Science 1 1%
Mathematics 1 1%
Materials Science 1 1%
Unknown 5 7%
Attention Score in Context

Attention Score in Context

This research output has an Altmetric Attention Score of 4. 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 22 January 2024.
All research outputs
#7,210,869
of 23,524,722 outputs
Outputs from ADS
#8,911
of 38,166 outputs
Outputs of similar age
#46,585
of 170,525 outputs
Outputs of similar age from ADS
#250
of 829 outputs
Altmetric has tracked 23,524,722 research outputs across all sources so far. This one has received more attention than most of these and is in the 68th percentile.
So far Altmetric has tracked 38,166 research outputs from this source. They receive a mean Attention Score of 4.6. This one has done well, scoring higher than 75% of its peers.
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 170,525 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 71% of its contemporaries.
We're also able to compare this research output to 829 others from the same source and published within six weeks on either side of this one. This one has gotten more attention than average, scoring higher than 67% of its contemporaries.