NGC 6365

Last updated
NGC 6365
N6365s.jpg
Observation data
Constellation Draco (constellation)
Right ascension 17h 22m 43.7s
Declination 62° 10′ 12″
Apparent magnitude  (V)13.9 and 14.2
Apparent magnitude  (B)14.6 and 14,8
Surface brightness 14.00 and 12.56 mag/am2
Characteristics
Type Interacting galaxies
Other designations
CGCG 300-20

VV 232 Arp 30 NGC 6365A PGC 60174 UGC 10832 MCG 10-25-19 KCPG 511A NGC 6365B PGC 60171 CGCG 10833 MCG 10-25-18 KCPG 511B

IRAS 17222+6212

Contents

NGC 6365 is a pair of spiral galaxies in the constellation Draco. It consists of two galaxies, PGC 60174 to the south, and PGC 60171 to the north. These two galaxies are also designated respectively by the NASA/IPAC database as NGC 6365A [1] and NGC 6365B. [2] This pair of galaxies was discovered by German astronomer Lewis Swift in 1884. [3]

NGC 6563A

NGC 6563A is the northern counterpart of NGC 6563, and is a barred spiral galaxy. Its coordinates are 17h 22m 43.8s and 62° 09′ 57.9″. [3] Its speed relative to the cosmic microwave background is 8,413 ± 4 km/s, which corresponds to a Hubble distance of 124.1 ± 8.7 Mpc (~405 million ly). [3]

The luminosity class of NGC 6365A is III-IV and it has a broad HI [3] line. It is an active galaxy (AGN) [4] of type Seyfert 2. [3]

With a surface brightness equal to 14.00 mag/am^2, we can qualify NGC 6365A as a low surface brightness galaxy (LSB). LSB galaxies are diffuse (D) galaxies with a surface brightness less than one magnitude lower than that of the ambient night sky.

To date, nearly fifteen measurements not based on redshift give a distance of 111.469 ± 31.088 Mpc (~364 million ly), [5] which is within the values of the Hubble distance.

Supernovae

Three supernovae have been observed in NGC 6365A:

NGC 6563B

NGC is the southern counterpart of NGC 6563, and is a spiral galaxy. However, the NASA/IPAC database indicates that it is Magellanic in type. Its coordinates are 17h 22m 43.5s and 62° 10′ 25.4″. [2] Its speed relative to the cosmic microwave background is 7,975 ± 4 km/s, which corresponds to a Hubble distance of 117.6 ± 8.2 Mpc (~384 million ly). [2] The luminosity class of NGC 6365B is IV-V and it has a broad HI line. It also contains regions of ionized hydrogen. [2]

Galaxy interaction

The pair of galaxies that make up NGC 6563 appear in Halton Arp's Atlas of Peculiar Galaxies under the designation Arp 30. Arp describes NGC 6365 as a spiral galaxy with an overdeveloped arm, but this has been recently confirmed by astronomers to be false. [9] In the image used by Arp, PGC 60171 (NGC 6365B) appears to be part of PGC 60174 and to be one galaxy. [9] But, they are actually two separate galaxies. According to redshift-based measurements, NGC 6365A is the most distant galaxy. However, given the uncertainties in the measurements, NGC 6365B could be the most distant galaxy. The image taken by the telescope at the Mount Lemmon observatory does not allow us to decide. There is no publication that is only speculative about their position and also about their interaction. [9]

See also

Related Research Articles

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<span class="mw-page-title-main">NGC 918</span> Barred spiral galaxy in the constellation Aries

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<span class="mw-page-title-main">NGC 7329</span> Galaxy in the constellation Tucana

NGC 7329 is a large barred spiral galaxy located in the constellation Tucana. NGC 7329 was discovered by British astronomer John Herschel in 1835.

<span class="mw-page-title-main">NGC 646</span> Galaxy in the constellation Hydrus

NGC 646 is a large barred spiral galaxy located in the constellation Hydrus. Its speed relative to the cosmic microwave background is 8,145 ± 19 km/s, which corresponds to a Hubble distance of 120.1 ± 8.4 Mpc. NGC 646 was discovered by British astronomer John Herschel in 1834. It forms an interacting galaxy pair.

<span class="mw-page-title-main">NGC 626</span> Galaxy in the constellation Sculptor

NGC 626 is a very large barred spiral galaxy located in the constellation Sculptor. Its speed relative to the cosmic microwave background is 5,475 ± 16 km/s, which corresponds to a Hubble distance of 80.8 ± 5.7 Mpc. NGC 626 was discovered by British astronomer John Herschel in 1834.

<span class="mw-page-title-main">NGC 3800</span> Galaxy in the constellation Leo

NGC 3800 is an intermediate spiral galaxy located in the constellation Leo. Its speed relative to the cosmic microwave background is 3,653 ± 24 km/s, which corresponds to a Hubble distance of 53.9 ± 3.8 Mpc. NGC 3800 was discovered by German-British astronomer William Herschel in 1784.

<span class="mw-page-title-main">NGC 3799</span> Galaxy in the constellation Leo

NGC 3799 is a barred spiral galaxy located in the constellation Leo. Its speed relative to the cosmic microwave background is 3,659 ± 24 km/s, which corresponds to a Hubble distance of 54.0 ± 3.8 Mpc. NGC 3799 was discovered by British astronomer John Herschel in 1832.

<span class="mw-page-title-main">NGC 5885</span> Barred spiral galaxy in the constellation Libra

NGC 5885 is an intermediate barred spiral galaxy located in the constellation Libra. Its speed relative to the cosmic microwave background is 2,185 ± 13 km/s, which corresponds to a Hubble distance of 32.3 ± 2.3 Mpc. NGC 5885 was discovered by German-British astronomer William Herschel in 1784.

<span class="mw-page-title-main">NGC 1024</span> Spiral galaxy in the constellation Aries

NGC 1024 is a large spiral galaxy of type Sab located in the constellation Aries. Its speed relative to the cosmic microwave background is 3,306 ± 16 km/s, which corresponds to a Hubble distance of 48.8 ± 3.4 Mpc. NGC 1024 was discovered by German-British astronomer William Herschel in 1786.

<span class="mw-page-title-main">NGC 4017</span> Spiral radio galaxy in the constellation Coma Berenices

NGC 4017 is an intermediate spiral radio galaxy located in the constellation Coma Berenices. Its speed relative to the cosmic microwave background is 3,748 ± 21 km/s, which corresponds to a Hubble distance of 55.3 ± 3.9 Mpc. NGC 4017 was discovered by German-British astronomer William Herschel in 1785.

<span class="mw-page-title-main">NGC 3200</span> Large galaxy in the constellation Hydra

NGC 3200 is a large spiral galaxy located in the constellation Hydra. Its velocity relative to the cosmic microwave background is 3,877 ± 25 km/s, which corresponds to a Hubble distance of 57.2 ± 4.0 Mpc. NGC 3200 was discovered by American astronomer Edward Singleton Holden in 1882.

<span class="mw-page-title-main">NGC 2648</span> Spiral galaxy in the constellation Cancer

NGC 2648 is a spiral galaxy located in the constellation Cancer. Its speed relative to the cosmic microwave background is 2,451 ± 19 km/s, which corresponds to a Hubble distance of 36.2 ± 2.6 Mpc. NGC 2648 was discovered by German-British astronomer William Herschel in 1784.

<span class="mw-page-title-main">NGC 5504</span> Spiral galaxy in the constellation Boötes

NGC 5504 is an intermediate barred spiral galaxy located in the constellation Boötes. Its speed relative to the cosmic microwave background is 5,482 ± 17 km/s, which corresponds to a Hubble distance of 80.9 ± 5.7 Mpc. NGC 5504 was discovered by French astronomer Édouard Stephan in 1880.

<span class="mw-page-title-main">NGC 7716</span> Spiral galaxy in the constellation Pisces

NGC 7716 is an intermediate spiral galaxy located in the constellation Pisces. Its speed relative to the cosmic microwave background is 2,201 ± 26 km/s, which corresponds to a Hubble distance of 32.5 ± 2.3 Mpc. NGC 7716 was discovered by British astronomer John Herschel in 1831.

<span class="mw-page-title-main">NGC 1320</span> Spiral galaxy in the constellation Eridanus

NGC 1320 is a spiral galaxy located in the constellation Eridanus. Its speed relative to the cosmic microwave background is 2,620 ± 15 km/s, which corresponds to a Hubble distance of 38.6 ± 2.7 Mpc. It was discovered by the German-British astronomer William Herschel in 1784.

<span class="mw-page-title-main">NGC 3447</span> Barred Magellanic spiral galaxy in the constellation Leo

NGC 3447 is a barred Magellanic spiral galaxy located in the constellation Leo. Its speed relative to the cosmic microwave background is 1,405 ± 34 km/s, which corresponds to a Hubble distance of 20.7 ± 1.5 Mpc. It was discovered by the British astronomer John Herschel in 1836.

<span class="mw-page-title-main">NGC 3187</span> Barred spiral galaxy in the constellation Leo

NGC 3187, also known as HGC 44D, is a large barred spiral galaxy located in the constellation Leo. Its velocity relative to the cosmic microwave background is 1,901 ± 22 km/s, which corresponds to a Hubble distance of 28.0 ± 2.0 Mpc. NGC 3187 was discovered by Irish physicist George Stoney in 1850.

<span class="mw-page-title-main">NGC 3177</span> Spiral galaxy in the constellation Leo

NGC 3177 is a spiral galaxy located in the constellation Leo. Its speed relative to the cosmic microwave background is 1,627 ± 22 km/s, which corresponds to a Hubble distance of 24.0 ± 1.7 Mpc. NGC 3177 was discovered by the German-British astronomer William Herschel in 1784.

<span class="mw-page-title-main">NGC 633</span> Large barred spiral galaxy in the constellation Sculptor

NGC 633 is a large barred spiral galaxy located in the constellation Sculptor. Its speed relative to the cosmic microwave background is 4,979 ± 18 km/s, which corresponds to a Hubble distance of 73.4 ± 5.2 Mpc. NGC 633 was discovered by British astronomer John Herschel in 1834.

<span class="mw-page-title-main">NGC 5394</span> Interacting barred spiral galaxy in the constellation Canes Venatici

NGC 5394 is a barred spiral galaxy located in the constellation Canes Venatici. Its speed relative to the cosmic microwave background is 3,639 ± 14 km/s, which corresponds to a Hubble distance of 53.7 ± 3.8 Mpc. NGC 5394 was discovered by German-British astronomer William Herschel in 1787.

References

  1. ↑ "By Name | NASA/IPAC Extragalactic Database". ned.ipac.caltech.edu. Retrieved 2024-05-09.
  2. 1 2 3 4 "By Name | NASA/IPAC Extragalactic Database". ned.ipac.caltech.edu. Retrieved 2024-05-09.
  3. 1 2 3 4 5 "By Name | NASA/IPAC Extragalactic Database". ned.ipac.caltech.edu. Retrieved 2024-05-09.
  4. ↑ "NGC 6365A". simbad.u-strasbg.fr. Retrieved 2024-05-09.
  5. ↑ "NED Query Results for NGC 6365A". ned.ipac.caltech.edu. Retrieved 2024-05-09.
  6. ↑ "Tom Boles searching for SuperNovae at the Coddenham Observatory". coddenhamobservatories.org. Retrieved 2024-05-09.
  7. ↑ "SN 2016ino". Transient Name Server. IAU . Retrieved 5 September 2024.
  8. ↑ "SN 2020qim". Transient Name Server. IAU . Retrieved 5 September 2024.
  9. 1 2 3 "New General Catalog Objects: NGC 6350 - 6399". cseligman.com. Retrieved 2024-05-09.
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