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Cool Stars, Stellar Systems, and the Sun

Overview of attention for book
Cover of 'Cool Stars, Stellar Systems, and the Sun'

Table of Contents

  1. Altmetric Badge
    Book Overview
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    Chapter 174 Recent observations of T Tauri stars
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    Chapter 175 Results from ultraviolet observations of T Tauri stars
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    Chapter 176 X-ray emission from pre-main sequence stars
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    Chapter 177 Infrared and molecular line observations of young stars and associated dense gas
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    Chapter 178 Photometric monitoring of T Tauri stars, RS CVn stars and related objects
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    Chapter 179 Angular momentum loss during pre-main sequence contraction
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    Chapter 180 Atmospheres and winds of T Tauri stars
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    Chapter 181 Post-T Taubi stars in T associations
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    Chapter 182 The formation of cool stars from cloud cores
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    Chapter 183 A dynamical origin for the stellar birthline
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    Chapter 184 Rotational velocities of low mass stars in intermediate age open clusters
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    Chapter 185 Measurements of rotational velocities of F and G stars
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    Chapter 186 High-resolution observations of cool stars with the ESO Coude' Echelle Spectrometer
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    Chapter 187 The rapidly-rotating field M-dwarf Gliese 890
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    Chapter 188 Evolution of rotation in main-sequence stars
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    Chapter 189 On the origins of chromospheric activity in late-type stars
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    Chapter 190 Time series measurements of chromospheric emission and possible evidence for differential rotation
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    Chapter 191 Deterministic time series modeling of Ca II H & K stellar index data
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    Chapter 192 The evolution of coronal activity in main sequence cool stars
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    Chapter 193 Coronal structure and rotation in late-type stars
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    Chapter 194 A search for secular luminosity variations in the Pleiades cluster
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    Chapter 195 Solar flux variations and concepts for a stellar photometric satellite
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    Chapter 196 Solar-cycle temperature variations in sunspots
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    Chapter 197 HRTS ultraviolet images of the solar chromosphere and transition zone
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    Chapter 198 The NSO initiative to pursue the solar-stellar connection on the McMath Solar Telescope
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    Chapter 199 Laboratory identification of the 3 P 1,2 - 5 S 2 O intersystem lines of S III
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    Chapter 200 Transition region — coronal models: A comparison with XUV observations
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    Chapter 201 X-ray transients and flares from active stellar systems
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    Chapter 202 Long-term behavior of stellar flare activity in AD Leo
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    Chapter 203 Radio observations of active stars: Direct evidence for polarity reversals?
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    Chapter 204 Capella HL
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    Chapter 205 Lithium depletion in solar-type stars
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    Chapter 206 Nitrogen abundances in disk and halo dwarfs
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    Chapter 207 Four W ursae majoris contact binaries in the old galactic cluster NGC 188
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    Chapter 208 Does the physical state of a mantle indicate the stage of evolution of a star?
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    Chapter 209 A review of the first observations of stars using the Infrared Astronomical Satellite (IRAS)
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    Chapter 210 RS CVn binary systems
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    Chapter 211 Starspots, differential rotation and a possible six-year spot cycle on Lambda Andromedae
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    Chapter 212 Visual and infrared photometry of the long-period RS CVn system HR 7275
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    Chapter 213 Hα observations of the RS CVn star, RT LAC: Evidence for gas streaming: Preliminary results
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    Chapter 214 Near infrared photometry of some RS CVn systems
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    Chapter 215 The puzzle of the UV continua of the Hyades giants
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    Chapter 216 Multicolor photometry of the active G giant FK Com
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    Chapter 217 Rotational modulation and high speed streams in FK Comae Berenices: Evidence for a massive, highly-evolved binary system
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    Chapter 218 Outer atmospheres of giant and supergiant stars
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    Chapter 219 Envelopes of red giant stars
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    Chapter 220 Radiative transfer in an expanding spherical medium
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    Chapter 221 Asymptotic giant branch stars as producers of carbon and of neutron-rich isotopes
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    Chapter 222 Chromospheres in metal deficient field stars
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    Chapter 223 Interpretation of the observed MG II emission from N-type carbon stars
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    Chapter 224 Introductory remarks to the session on alpha orionis and related topics
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    Chapter 225 Multiband photoelectric photometry of Betelgeuse
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    Chapter 226 Lower atmospheric changes in Betelgeuse deduced from optical continua polarization measurements
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    Chapter 227 Photoionization of the circumstellar shell of Betelgeuse by chromospheric radiation
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    Chapter 228 Better determinations of mass loss rates for red giants and supergiants
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    Chapter 229 Sulphur I emission lines in the EUV spectrum of β GRU (M3 II)
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    Chapter 230 OH maser emission as a probe of circumstellar envelope structure
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    Chapter 231 Preliminary results from studies of high resolution line spectra of late-type giant and supergiant stars
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    Chapter 232 Discovery of a hot, interactive companion to the S star HD 35155
Overall attention for this book and its chapters
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About this Attention Score

  • In the top 25% of all research outputs scored by Altmetric
  • High Attention Score compared to outputs of the same age (93rd percentile)
  • High Attention Score compared to outputs of the same age and source (97th percentile)

Mentioned by

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1 blog
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2 X users
wikipedia
10 Wikipedia pages

Readers on

mendeley
6 Mendeley
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Title
Cool Stars, Stellar Systems, and the Sun
Published by
ADS, January 2006
DOI 10.1007/3-540-12907-3
ISBNs
978-3-54-012907-3, 978-3-54-038785-5
Editors

Baliunas, Sallie L., Hartmann, Lee

X Demographics

X Demographics

The data shown below were collected from the profiles of 2 X users 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 6 Mendeley readers of this research output. Click here to see the associated Mendeley record.

Geographical breakdown

Country Count As %
Canada 1 17%
Unknown 5 83%

Demographic breakdown

Readers by professional status Count As %
Student > Ph. D. Student 3 50%
Student > Master 2 33%
Researcher 1 17%
Readers by discipline Count As %
Physics and Astronomy 6 100%
Attention Score in Context

Attention Score in Context

This research output has an Altmetric Attention Score of 12. 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 April 2024.
All research outputs
#2,638,084
of 23,041,514 outputs
Outputs from ADS
#1,705
of 37,451 outputs
Outputs of similar age
#9,435
of 156,480 outputs
Outputs of similar age from ADS
#10
of 436 outputs
Altmetric has tracked 23,041,514 research outputs across all sources so far. Compared to these this one has done well and is in the 88th percentile: it's in the top 25% of all research outputs ever tracked by Altmetric.
So far Altmetric has tracked 37,451 research outputs from this source. They receive a mean Attention Score of 4.6. This one has done particularly well, scoring higher than 95% 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 156,480 tracked outputs that were published within six weeks on either side of this one in any source. This one has done particularly well, scoring higher than 93% of its contemporaries.
We're also able to compare this research output to 436 others from the same source and published within six weeks on either side of this one. This one has done particularly well, scoring higher than 97% of its contemporaries.