NGC 7343

Last updated • 1 min readFrom Wikipedia, The Free Encyclopedia
NGC 7343
NGC7343 - SDSS DR14.jpg
NGC 7343 imaged by the Sloan Digital Sky Survey
Observation data (J2000 epoch)
Constellation Pegasus
Right ascension 22h 38m 37.8618s [1]
Declination +34° 04′ 17.307″ [1]
Apparent magnitude  (V)13.5
Apparent magnitude  (B)14.4
Surface brightness 13.26 mag/arcsec2
Characteristics
Size~90,500  ly (27.75  kpc) (estimated) [1]
Other designations
IRAS 22363+3348, UGC 12129, MCG +06-49-059, PGC 69391, CGCG 514-082 [1]

NGC 7343 is a barred spiral galaxy located in the constellation Pegasus. Its velocity relative to the cosmic microwave background is 7150 ± 24 km/s, which corresponds to a Hubble distance of 105.5 ± 7.4 Mpc (∼344 million ly). NGC 7343 was discovered by American astronomer Truman Safford in 1866. It was independently rediscovered by French astronomer Édouard Stephan on September 27, 1873.

Contents

The luminosity class of NGC 7343 is II-III and it has a broad HI line. In addition, it is also a LINER galaxy, a galaxy whose nucleus presents an emission spectrum characterized by broad lines of weakly ionized atoms. To date, eight non-redshift measurements yield a distance of 65.787 ± 44.256 Mpc (∼215 million ly), which is outside the Hubble distance values. [2] [3] [1] [4] [5]

Supernova

The supernova SN 1974J (type Ia, mag. 15.5) was discovered in NGC 7343 on 9 October 1974 by Italian astronomer Leonida Rosino. [6] [7]

See also

Related Research Articles

<span class="mw-page-title-main">NGC 2441</span> Galaxy in the constellation Camelopardalis

NGC 2441 is a barred spiral galaxy located in the northern constellation of Camelopardalis. Its velocity with respect to the cosmic microwave background is 3492 ± 2 km/s, which corresponds to a Hubble distance of 168.0 ± 11.8 Mly (51.51 ± 3.61 Mpc). In addition, 16 non-redshift measurements give a distance of 176.16 ± 16.80 Mly (54.012 ± 5.151 Mpc). The galaxy was discovered by German astronomer Wilhelm Tempel on 8 August 1882.

<span class="mw-page-title-main">NGC 2300</span> Galaxy in the constellation Cepheus

NGC 2300 is a lenticular galaxy in the constellation Cepheus. Its velocity with respect to the cosmic microwave background is 1876 ± 7 km/s, which corresponds to a Hubble distance of 90.2 ± 6.3 Mly (27.67 ± 1.94 Mpc). However, 11 non redshift measurements give a distance of 131.98 ± 21.75 Mly (40.464 ± 6.668 Mpc). The galaxy was discovered in 1871 by French astronomer Alphonse Borrelly using an 18 cm telescope.

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

NGC 918 is a barred spiral galaxy in the constellation Aries, about 67 million light years from the Milky Way. It was discovered by John Herschel on Jan 11, 1831.

<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 6365</span> Galaxy pair in the constellation Draco

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 and NGC 6365B. This pair of galaxies was discovered by German astronomer Lewis Swift in 1884.

<span class="mw-page-title-main">NGC 2935</span> Large galaxy in constellation Hydra

NGC 2935 is a large intermediate spiral galaxy located in the constellation Hydra. Its speed relative to the cosmic microwave background is 2,601 ± 23 km/s, which corresponds to a Hubble distance of 38.4 ± 2.7 Mpc. It was discovered by German-British astronomer William Herschel on 20 March 1786.

<span class="mw-page-title-main">NGC 4712</span> Spiral galaxy in the constellation Coma Berenices

NGC 4712 is a spiral galaxy located in the constellation Coma Berenices. Its speed relative to the cosmic microwave background is 4,664 ± 20 km/s, which corresponds to a Hubble distance of 68.8 ± 4.8 Mpc. NGC 4712 was discovered by German-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 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 1175</span> Large lenticular galaxy in the constellation Perseus

NGC 1175, also known as the Peanut Galaxy, is a large lenticular galaxy located in the constellation Perseus. Its speed relative to the cosmic microwave background is 5,349 ± 19 km/s, which corresponds to a Hubble distance of 78.9 ± 5.5 Mpc. It was discovered by the German-British astronomer William Herschel in 1786.

<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 5416</span> Spiral and radio galaxy in the constellation Boötes

NGC 5416 is a spiral galaxy and radio galaxy located in the constellation Boötes. Its speed relative to the cosmic microwave background is 6,499 ± 18 km/s, which corresponds to a Hubble distance of 95.9 ± 6.7 Mpc. NGC 5416 was discovered by 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 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 5377</span> Intermediate barred spiral galaxy in the constellation Canes Venatici

NGC 5377 is an intermediate barred spiral galaxy located in the constellation Canes Venatici. Its speed relative to the cosmic microwave background is 1,951 ± 11 km/s, which corresponds to a Hubble distance of 28.8 ± 2.0 Mpc. NGC 5377 was discovered by German-British astronomer William Herschel in 1787.

<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. 1 2 3 4 5 "Results for object NGC 7343". NASA/IPAC Extragalactic Database. NASA and Caltech . Retrieved 7 December 2024.
  2. ↑ "Your NED Search Results, Distance Results for NGC 7343". ned.ipac.caltech.edu. Retrieved 2024-08-11.
  3. ↑ "Les données de "Revised NGC and IC Catalog by Wolfgang Steinicke", NGC 7300 à 7399" (in French). Site WEB du cours d'astronomie du Cégep de Valleyfield.
  4. ↑ Courtney Seligman. "Celestial Atlas Table of Contents, NGC 7300 à 7349" . Retrieved December 5, 2024..
  5. ↑ "NGC 7343 sur HyperLeda" . Retrieved December 5, 2024.
  6. ↑ Rosino, L. (1974). "Supernova in NGC 7343". International Astronomical Union Circular (2707): 1. Bibcode:1974IAUC.2707....1R.
  7. ↑ "SN 1974J". Transient Name Server. IAU . Retrieved 7 December 2024.
This page is based on this Wikipedia article
Text is available under the CC BY-SA 4.0 license; additional terms may apply.
Images, videos and audio are available under their respective licenses.