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Sub-brown dwarf and WD 0806-661

Shortcuts: Differences, Similarities, Jaccard Similarity Coefficient, References.

Difference between Sub-brown dwarf and WD 0806-661

Sub-brown dwarf vs. WD 0806-661

A sub-brown dwarf or planetary-mass brown dwarf is an astronomical object that formed in the same manner as stars and brown dwarfs (i.e. through the collapse of a gas cloud) but that has a mass below the limiting mass for thermonuclear fusion of deuterium (about). Some researchers call them free-floating planets whereas others call them planetary-mass brown dwarfs. WD 0806-661 (L 97-3, GJ 3483) is a wide binary system of a white dwarf and a Y-type sub-brown dwarf (designated "B"), located in constellation Volans at 63 light-years from Earth.

Similarities between Sub-brown dwarf and WD 0806-661

Sub-brown dwarf and WD 0806-661 have 2 things in common (in Unionpedia): DT Virginis, The Astrophysical Journal.

DT Virginis

DT Virginis, also known as Ross 458 AB, is a binary star in the constellation of Virgo.

DT Virginis and Sub-brown dwarf · DT Virginis and WD 0806-661 · See more »

The Astrophysical Journal

The Astrophysical Journal, often abbreviated ApJ (pronounced "ap jay") in references and speech, is a peer-reviewed scientific journal of astrophysics and astronomy, established in 1895 by American astronomers George Ellery Hale and James Edward Keeler.

Sub-brown dwarf and The Astrophysical Journal · The Astrophysical Journal and WD 0806-661 · See more »

The list above answers the following questions

Sub-brown dwarf and WD 0806-661 Comparison

Sub-brown dwarf has 25 relations, while WD 0806-661 has 19. As they have in common 2, the Jaccard index is 4.55% = 2 / (25 + 19).

References

This article shows the relationship between Sub-brown dwarf and WD 0806-661. To access each article from which the information was extracted, please visit:

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