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Magellanic spiral

Index Magellanic spiral

Magellanic spiral galaxies are (usually) dwarf galaxies which are classified as the type Sm (and SAm, SBm, SABm). [1]

31 relations: Barred spiral galaxy, David Dunlap Observatory Catalogue, Density wave theory, Dwarf galaxy, Dwarf spiral galaxy, Galaxy morphological classification, Intermediate spiral galaxy, Irregular galaxy, Large Magellanic Cloud, Magellanic, Magellanic Clouds, NGC 2363, NGC 2552, NGC 3109, NGC 4449, NGC 4523, NGC 4618, NGC 4625, NGC 5002, NGC 5204, NGC 55, NGC 5713, NGC 925, Outline of galaxies, Sam, SBM, SM, UGC 5692, UGCA 1, UGCA 86, Unbarred spiral galaxy.

Barred spiral galaxy

A barred spiral galaxy is a spiral galaxy with a central bar-shaped structure composed of stars.

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David Dunlap Observatory Catalogue

David Dunlap Observatory Catalogue, known as the DDO or A Catalogue of Dwarf Galaxies, is a catalogue of dwarf galaxies that was published in 1959 (and later expanded in 1966) by Sidney van den Bergh.

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Density wave theory

Density wave theory or the Lin-Shu density wave theory is a theory proposed by C.C. Lin and Frank Shu in the mid-1960s to explain the spiral arm structure of spiral galaxies.

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Dwarf galaxy

A dwarf galaxy is a small galaxy composed of about 100 million up to several billion stars, a small number compared to the Milky Way's 200–400 billion stars.

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Dwarf spiral galaxy

A dwarf spiral galaxy is the dwarf version of a spiral galaxy.

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Galaxy morphological classification

Galaxy morphological classification is a system used by astronomers to divide galaxies into groups based on their visual appearance.

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Intermediate spiral galaxy

An intermediate spiral galaxy is a galaxy that is in between the classifications of a barred spiral galaxy and an unbarred spiral galaxy.

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Irregular galaxy

An irregular galaxy is a galaxy that does not have a distinct regular shape, unlike a spiral or an elliptical galaxy.

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Large Magellanic Cloud

The Large Magellanic Cloud (LMC) is a satellite galaxy of the Milky Way.

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Magellanic

Magellanic may refer to.

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Magellanic Clouds

The Magellanic Clouds (or Nubeculae Magellani) are two irregular dwarf galaxies visible in the Southern Celestial Hemisphere; they are members of the Local Group and are orbiting the Milky Way galaxy.

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NGC 2363

NGC 2363 is a star-forming region in the Magellanic galaxy NGC 2366 which is located in the constellation Camelopardalis.

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NGC 2552

NGC 2552 is a Magellanic spiral galaxy located some 22 million light years away in the faint northern constellation of Lynx.

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NGC 3109

NGC 3109 is a small barred Magellanic type spiral or irregular galaxy around 4.2 Mly away in the direction of the constellation of Hydra.

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NGC 4449

NGC 4449 is an irregular Magellanic type galaxy in the constellation Canes Venatici, being located about 12 million light-years away.

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NGC 4523

NGC 4523 is a Magellanic spiral galaxy located about 35 to 50 million light-years away in the constellation Coma Berenices.

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NGC 4618

NGC 4618 is a distorted barred dwarf galaxy in the constellation Canes Venatici.

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NGC 4625

NGC 4625 is a distorted dwarf galaxy in the constellation Canes Venatici.

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NGC 5002

NGC 5002 is a Magellanic spiral galaxy in Canes Venatici.

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NGC 5204

NCG 5204 is a Magellanic spiral galaxy located about 14.5 million light-years away from EarthThe distance from Earth is.

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NGC 55

NGC 55, also occasionally referred to as The Whale Galaxy, is a Magellanic type barred spiral galaxy located about 7 million light-years away in the constellation Sculptor.

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NGC 5713

NGC 5713 is a peculiar, asymmetric galaxy in the constellation Virgo.

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NGC 925

NGC 925 is a barred spiral galaxy located about 30 million light-years away in the constellation Triangulum.

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Outline of galaxies

The following outline is provided as an overview of and topical guide to galaxies: Galaxies – gravitationally bound systems of stars, stellar remnants, interstellar gas, dust, and dark matter.

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Sam

Sam, SAM or variants may refer to.

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SBM

SBM may stand for.

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SM

SM or sm may refer to.

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UGC 5692

UGC 5692 is a Magellanic-type spiral galaxy located 13 million light years away in the constellation of Ursa Major.

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UGCA 1

UGCA 1, also known as PGC 538 is a Magellanic barred spiral galaxy located about 160 million light-years away in the constellation Cetus.

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UGCA 86

UGCA 86 is a Magellanic spiral galaxy.

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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.

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Redirects here:

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References

[1] https://en.wikipedia.org/wiki/Magellanic_spiral

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