NGC 3511

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NGC 3511
NGC 3511 PanSTARRS1 i.g.jpg
NGC 3511 by PanSTARRS
Observation data (J2000 epoch)
Constellation Crater
Right ascension 11h 03m 23.8s [1]
Declination −23° 05 12 [1]
Redshift 0.003699 ± 0.000010 [1]
Heliocentric radial velocity 1,109 ± 3 km/s [1]
Distance 41.5 ± 6.4 Mly (12.7 ± 2.0 Mpc) [1]
Apparent magnitude  (V)10.8 [2]
Characteristics
Type SAB(s)c [1]
Apparent size  (V)5.8 × 2.0
Notable featuresExtended HIPASS source [1]
Other designations
UGCA 223, ESO 502- G013, AM 1100-224, MCG -04-26-020, PGC 33385 [1]

NGC 3511 is an intermediate spiral galaxy located in the constellation Crater. It is located at a distance of circa 45 million light years from Earth, which, given its apparent dimensions, means that NGC 3511 is about 70,000 light years across. It was discovered by William Herschel on December 21, 1786. [3] It lies two degrees west of Beta Crateris. [4]

Contents

NGC 3511 features two very diffuse, thick, and patchy spiral arms that emanate from the bulge, while there are also other spiral arm fragments. Dark dust lanes can be seen across the spiral pattern. The bulge appears elliptical and is weak. [5] The galaxy is seen at a high inclination, estimated to be 70°. [6] In the centre of the galaxy lies a supermassive black hole, whose mass is estimated to be 106.46 ± 0.33 (1.3 - 6.2 million) M, based on the pitch angle of the spiral arms. [7] The galaxy had been classified as a type 1 Seyfert galaxy, [8] however it features only narrow emission lines, and has been reclassified as a HII region galaxy. [9] The Infrared Spectrograph (IRS) on the Spitzer Space Telescope has detected polycyclic aromatic hydrocarbon (PAH) emission. [10]

NGC 3511 forms a pair with NGC 3513, which lies 10.5 arcminutes away from NGC 3511. [11] The two galaxies form a small group, known as the NGC 3511 group, which also includes the galaxy ESO 502-024. [12]

See also

Related Research Articles

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<span class="mw-page-title-main">NGC 1964</span> Galaxy in the constellation Lepus

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<span class="mw-page-title-main">NGC 4237</span> Galaxy in the constellation Coma Berenices

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<span class="mw-page-title-main">NGC 3367</span> Spiral galaxy in the constellation Leo

NGC 3367 is a barred spiral galaxy located in the constellation Leo. It is located at a distance of about 120 million light years from Earth, which, given its apparent dimensions, means that NGC 3367 is about 85,000 light years across. It was discovered by William Herschel on March 19, 1784.

<span class="mw-page-title-main">NGC 4939</span> Spiral galaxy in the constellation Virgo

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<span class="mw-page-title-main">NGC 4636</span> Galaxy in the constellation Virgo

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<span class="mw-page-title-main">NGC 7531</span> Galaxy in the constellation Grus

NGC 7531 is an intermediate spiral galaxy located in the constellation Grus. It is located at a distance of about 70 million light-years from Earth, which, given its apparent dimensions, means that NGC 7531 is about 95,000 light years across. It was discovered by John Herschel on September 2, 1836.

<span class="mw-page-title-main">NGC 7418</span> Galaxy in the constellation Grus

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<span class="mw-page-title-main">NGC 4074</span> Galaxy in the constellation Coma Berenices

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<span class="mw-page-title-main">NGC 2525</span> Galaxy in the constellation Puppis

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<span class="mw-page-title-main">NGC 4302</span> Galaxy in the constellation Coma Berenices

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<span class="mw-page-title-main">NGC 1241</span> Galaxy in the constellation Eridanus

NGC 1241 is a spiral galaxy located in the constellation Eridanus. It is located at a distance of circa 150 million light years from Earth, which, given its apparent dimensions, means that NGC 1241 is about 140,000 light years across. It was discovered by William Herschel on January 10, 1785. It is classified as a Seyfert galaxy.

<span class="mw-page-title-main">NGC 7592</span> Interacting galaxy system in the constellation Aquarius

NGC 7592 is an interacting galaxy system located 300 million light years away in the constellation Aquarius. It was discovered by William Herschel on September 20, 1784. The total infrared luminosity is 1011.33 L, and thus it is categorised as a luminous infrared galaxy. One of the galaxies hosts a type 2 Seyfert nucleus.

<span class="mw-page-title-main">NGC 5273</span> Galaxy in the constellation Canes Venatici

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References

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