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Home » Articles » Linux » Here
This article discusses the archiving tools available in Linux, with specific reference to the information needed for the RHCSA EX200 and RHCE EX300 certification exams.
Remember, the exams are hands-on, so it doesn't matter which method you use to achieve the result, so long as the end product is correct.
All the commands in this article have many options in addition to the basic ones being used here. Please check the man pages for each command. The examples will use the following files.
Extracts assume the '/tmp/extract-dir' directory is empty.
tar
Create an archive.
Check the contents.
Extract it.
star
The star command may not be installed by default, but you can install it with the following command.
Create an archive.
Check the contents.
Extract it.
gzip
Binary Star Zippy
The gzip command compresses the specified files, giving them a '.gz' extension. In this case we will use it to compress a '.tar' file.
Binary Star Music Group
The '-z' option of the tar command allows you to do this directly.
The files are uncompressed using the gunzip command.
The '-z' option of the tar command allows you to directly ungzip and extract a '.tar.gz' file.
bzip2
The bzip2 command is similar to the gzip command. It compresses the specified files, giving them a '.bz2' extension. In this case we will use it to compress a '.tar' file.
The '-j' option of the tar command allows you to do this directly.
The files are uncompressed using the bunzip2 command.
The '-j' option of the tar command allows you to directly bunzip2 and extract a '.tar.bz2' file.
zip
Create an archive.
Check the contents.
Extract it.
cpio
Create an archive.
Check the contents.
Extract it.
For more information see:
Hope this helps. Regards Tim..
Learning Goals: Students will learn how the changing light from an eclipsing binary star system can reveal information about the individual stars and their orbits.
Sims 4 lights cc outdoor. Suggested Observations: time-delay series of images of a known eclipsing binary star system timed during subsequent minima (the dimmest point in the lightcurve) e.g.: AB And, BU Vul, XZ And
Challenge:
Find the period and relative luminosities of the components of an eclipsing binary star system. Observe an eclipsing binary and make a measurement of its period.
Part 1: Occulting Stars
Part 3: Period of an Eclipsing Binary
Resources: Worksheet
Terminology:binary star, lightcurve, minimum
Demos from UNL: Eclipsing Binary
Tutorials: Importing Images into MaxIm, Photometry in Maxim
Background:
A binary star is a star system consisting of two stars orbiting around their common center of mass. The brighter star is called the primary and the other is its companion star, or secondary. Research between the early 19th century and today suggests that many stars are part of either binary star systems or star systems with more than two stars, called multiple star systems. The term double star may be used synonymously with binary star, but more generally, a double star may be either a binary star or an optical double star which consists of two stars with no physical connection but which appear close together in the sky as seen from the Earth. A double star may be determined to be optical if its components have sufficiently different proper motions or radial velocities, or if parallax measurements reveal its two components to be at sufficiently different distances from the Earth. Most known double stars have not yet been determined to be either bound binary star systems or optical doubles.
Binary star systems are very important in astrophysics because calculations of their orbits allow the masses of their component stars to be directly determined, which in turn allows other stellar parameters, such as radius and density, to be indirectly estimated. This also determines an empirical mass-luminosity relationship (MLR) from which the masses of single stars can be estimated.
Create an archive.
Check the contents.
Extract it.
star
The star command may not be installed by default, but you can install it with the following command.
Create an archive.
Check the contents.
Extract it.
gzip
Binary Star Zippy
The gzip command compresses the specified files, giving them a '.gz' extension. In this case we will use it to compress a '.tar' file.
Binary Star Music Group
The '-z' option of the tar command allows you to do this directly.
The files are uncompressed using the gunzip command.
The '-z' option of the tar command allows you to directly ungzip and extract a '.tar.gz' file.
bzip2
The bzip2 command is similar to the gzip command. It compresses the specified files, giving them a '.bz2' extension. In this case we will use it to compress a '.tar' file.
The '-j' option of the tar command allows you to do this directly.
The files are uncompressed using the bunzip2 command.
The '-j' option of the tar command allows you to directly bunzip2 and extract a '.tar.bz2' file.
zip
Create an archive.
Check the contents.
Extract it.
cpio
Create an archive.
Check the contents.
Extract it.
For more information see:
Hope this helps. Regards Tim..
Learning Goals: Students will learn how the changing light from an eclipsing binary star system can reveal information about the individual stars and their orbits.
Sims 4 lights cc outdoor. Suggested Observations: time-delay series of images of a known eclipsing binary star system timed during subsequent minima (the dimmest point in the lightcurve) e.g.: AB And, BU Vul, XZ And
Challenge:
Find the period and relative luminosities of the components of an eclipsing binary star system. Observe an eclipsing binary and make a measurement of its period.
Part 1: Occulting Stars
Part 3: Period of an Eclipsing Binary
Resources: Worksheet
Terminology:binary star, lightcurve, minimum
Demos from UNL: Eclipsing Binary
Tutorials: Importing Images into MaxIm, Photometry in Maxim
Background:
A binary star is a star system consisting of two stars orbiting around their common center of mass. The brighter star is called the primary and the other is its companion star, or secondary. Research between the early 19th century and today suggests that many stars are part of either binary star systems or star systems with more than two stars, called multiple star systems. The term double star may be used synonymously with binary star, but more generally, a double star may be either a binary star or an optical double star which consists of two stars with no physical connection but which appear close together in the sky as seen from the Earth. A double star may be determined to be optical if its components have sufficiently different proper motions or radial velocities, or if parallax measurements reveal its two components to be at sufficiently different distances from the Earth. Most known double stars have not yet been determined to be either bound binary star systems or optical doubles.
Binary star systems are very important in astrophysics because calculations of their orbits allow the masses of their component stars to be directly determined, which in turn allows other stellar parameters, such as radius and density, to be indirectly estimated. This also determines an empirical mass-luminosity relationship (MLR) from which the masses of single stars can be estimated.
Binary stars are often detected optically, in which case they are called visual binaries. Many visual binaries have long orbital periods of several centuries or millennia and therefore have orbits which are uncertain or poorly known. They may also be detected by indirect techniques, such as spectroscopy (spectroscopic binaries) or astrometry (astrometric binaries). If a binary star happens to orbit in a plane along our line of sight, its components will eclipse and transit each other; these pairs are called eclipsing binaries, or, as they are detected by their changes in brightness during eclipses and transits, photometric binaries.
