Unbarred spiral galaxy

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Short description: Type of spiral galaxy without a central bar
The Whirlpool Galaxy and its companion satellite. The Whirlpool is an unbarred spiral galaxy.

An unbarred spiral galaxy is a type of spiral galaxy without a central bar, or one that is not a barred spiral galaxy. It is designated with an SA in the galaxy morphological classification scheme. A nearby example of an unbarred spiral is the Triangulum Galaxy.

Unbarred spiral galaxies are one of three general types of spiral galaxies under the de Vaucouleurs classification system, the other two being intermediate spiral galaxy and barred spiral galaxy. Under the Hubble tuning fork, it is one of two general types of spiral galaxy, the other being barred spirals.[1][2]

Overview

Roughly one third of known spiral galaxies are unbarred. Spiral galaxies range in diameter from about 20,000 to over 100,000 light-years; smaller spiral galaxies are less likely to have a stable bar than larger ones.[3] Unbarred spiral galaxies tend to have a higher redshift and are older than barred spirals, suggesting they represent an earlier stage in galactic evolution. The ratio of unbarred to barred spiral galaxies has fallen over the history of the universe.[4]

Classification

Under the de Vaucouleurs classification system, SA galaxies are one of three types of spiral galaxy.

In 1926, Edwin Hubble introduced the Hubble sequence for morphological classification of galaxies. Spiral galaxies, defined by their disc shape and presence of star-forming spiral arms, were divided into unbarred (SA) and barred (SB) types. Both types were further subdivided along a continuum of how tightly wound their spiral arms were, from tightly to loosely (a–c).[3][5]

Gérard de Vaucouleurs further expanded on this system in 1959. He described an intermediate class of spiral galaxy (SAB), between barred and unbarred, that shared features of both. He noted the continuity between loosely wound spiral galaxies and Magellanic spirals (galaxies with only one spiral arm), which he assigned the classes Sd and Sm. He also introduced classes for a galaxy's inner structure, sorted by whether the arms originated from a central ringlike structure or were purely spiral, allowing for mixed types: (r), (rs), (sr), and (s).[6]

Example Type Image Information Notes
SA0- SA0- is a type of lenticular galaxy
SA0 SA0 is a type of lenticular galaxy
SA0+ SA0+ is a type of lenticular galaxy
NGC 3593 SA0/a 100px SA0/a can also be considered a type of unbarred lenticular galaxy NGC 3593 is an "SA(s)0/a"
NGC 3169 SAa 100px NGC 3169 is an "SA(s)a pec"
Messier 81 SAab 100px M81 is an "SA(s)ab"
Messier 88 SAb 100px M88 is an "SA(rs)b"
NGC 3949 SAbc 100px NGC 3949 is an "SA(s)bc"
NGC 4414 SAc 100px NGC 4414 is an "SA(rs)c"
Triangulum Galaxy SAcd 100px Triangulum is an "SA(s)cd"
NGC 300 SAd 100px NGC 300 is an "SA(s)d"
NGC 45 SAdm 100px SAdm can also be considered a type of unbarred Magellanic spiral NGC 45 is an "SA(s)dm"
NGC 4395 SAm 100px SAm is a type of Magellanic spiral (Sm) NGC 4395 is an "SA(s)m"
An example of this type, imaged by the Hubble Space Telescope

Unbarred lenticular galaxy

An unbarred lenticular galaxy is a lenticular version of an unbarred spiral galaxy. They have the Hubble type of SA0.


References




Licensed under CC BY-SA 3.0 | Source: https://handwiki.org/wiki/Astronomy:Unbarred_spiral_galaxy
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