Energy output and surface termperature for Star Cluster CYG OB1.
Usage
data("CYGOB1")
Format
A data frame with 47 observations on the following 2 variables.
logst
log survface termperature of the star.
logli
log light intensity of the star.
Details
The Hertzsprung-Russell (H-R) diagram forms the basis of
the theory of stellar evolution. The diagram is essentially a
plot of the energy output of stars plotted against their surface
temperature. Data from the H-R diagram of Star Cluster CYG OB1,
calibrated according to VanismaGreve1972 are given here.
Source
F. Vanisma and J. P. De Greve (1972), Close binary systems
before and after mass transfer. Astrophysics and Space Science,
87, 377–401.
D. J. Hand, F. Daly, A. D. Lunn, K. J. McConway and E. Ostrowski (1994).
A Handbook of Small Datasets, Chapman and Hall/CRC, London.
Examples
data("CYGOB1", package = "HSAUR2")
plot(logst ~ logli, data = CYGOB1)
Results
R version 3.3.1 (2016-06-21) -- "Bug in Your Hair"
Copyright (C) 2016 The R Foundation for Statistical Computing
Platform: x86_64-pc-linux-gnu (64-bit)
R is free software and comes with ABSOLUTELY NO WARRANTY.
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Type 'license()' or 'licence()' for distribution details.
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'citation()' on how to cite R or R packages in publications.
Type 'demo()' for some demos, 'help()' for on-line help, or
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Type 'q()' to quit R.
> library(HSAUR2)
Loading required package: tools
> png(filename="/home/ddbj/snapshot/RGM3/R_CC/result/HSAUR2/CYGOB1.Rd_%03d_medium.png", width=480, height=480)
> ### Name: CYGOB1
> ### Title: CYG OB1 Star Cluster Data
> ### Aliases: CYGOB1
> ### Keywords: datasets
>
> ### ** Examples
>
>
> data("CYGOB1", package = "HSAUR2")
> plot(logst ~ logli, data = CYGOB1)
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> dev.off()
null device
1
>