IC 1192

Last updated
IC 1192
IC1192 - SDSS DR14.jpg
Sloan Digital Sky Survey image of IC 1192
Observation data
Constellation Hercules
Right ascension 16h 06m 33.130s
Declination +17d 46m 32.30s
Redshift 0.037936
Heliocentric radial velocity 11,373 km/s
Distance 543 Mly (166.4 Mpc)
Group or cluster Hercules Cluster
Apparent magnitude  (V)15.5
Characteristics
Type Sb, SBb, AGN
Size90,000 ly
Other designations
PGC 57157, SDSS J160633.12+174632.4, AGC 260226, USGC U741 NED06, ABELL 2151:[D80] 074, LEDA 57157

IC 1192 is an edge-on [1] barred spiral galaxy [2] located in Hercules. [3] [4] It is located 543 million light-years from the Solar System and has a diameter of approximately 90,000 light-years. [1] IC 1192 was discovered by Stephane Javelle on August 13, 1892. [5] It is a member of the Hercules Cluster. [6] [7]

The luminosity class of IC 1192 is II [1] and it has an active galaxy nucleus. It is specifically described as a LINER galaxy according to SIMBAD, meaning its nucleus presents an emission spectrum characterized by broad lines of weak ionized atoms. [8]

Related Research Articles

<span class="mw-page-title-main">NGC 4326</span> Barred spiral galaxy in the constellation of Virgo

NGC 4326 is a barred spiral galaxy with a ring located about 330 million light-years away in the constellation Virgo. It was discovered by astronomer William Herschel on April 13, 1784, who described it as "vF, S, R, bM, 1st of 3". It is a large galaxy, with a diameter of around 200,000 ly (61 kpc) making it nearly twice the size of the Milky Way. NGC 4326 is also classified as a LINER galaxy. Despite being listed in the Virgo Cluster catalog as VCC 623, it is not a member of the Virgo Cluster but instead a background galaxy.

<span class="mw-page-title-main">NGC 4333</span> Barred spiral galaxy in the constellation Virgo

NGC 4333 is a barred spiral galaxy with a ring structure located about 330 million light-years away in the constellation Virgo. It was discovered by astronomer William Herschel on April 13, 1784, who described it as "F, pS, R, bM, 2nd of 3". NGC 4333 is also classified as a LINER galaxy. Despite being listed in the Virgo Cluster catalog as VCC 637, it is not a member of the Virgo Cluster but instead a background galaxy.

<span class="mw-page-title-main">IC 3971</span> Spiral galaxy located in the constellation Coma Berenices

IC 3971 is a spiral galaxy located approximately 1 billion light-years away from the Solar System, in the constellation of Coma Berenices. It was first discovered in January 1904 by German astronomer Max Wolf. According to SIMBAD database, it is a LINER type galaxy with an active nucleus.

<span class="mw-page-title-main">IC 64</span> Galaxy in the constellation Pisces

IC 64 is a massive lenticular galaxy located 622 million light-years away in the Pisces constellation. IC 64 has a diameter of 300,000 thousand light-years, making it, three times bigger than the Milky Way and one of the largest galaxies observed. IC 64 was discovered by Stephane Javelle, a French astronomer on 5th December, 1893. It has an active galactic nucleus and is considered a radio galaxy.

<span class="mw-page-title-main">IC 5337</span> Galaxy in the constellation Pegasus

IC 5337 or JW100, is a spiral galaxy located 800 million light-years away from the Solar System in the constellation of Pegasus. It is probably gravitationally bound to IC 5338, the brightest cluster galaxy in Abell 2626. IC 5337 is a jellyfish galaxy, mainly due to dynamic stripping pressure. Star-forming gas are thrown about, as the galaxy penetrates through the thin gas layer and causing them to drip from the galaxy's disc, giving it its unique appearance of a cosmic jellyfish. In the image, other galaxies can be seen in the background.

<span class="mw-page-title-main">IC 3686</span> Galaxy in the constellation of Virgo

IC 3686 is a Sc type spiral galaxy located 920 million light-years from the Solar System in the constellation of Virgo. It was discovered by American astronomer, Royal Harwood Frost on May 10, 1904. Frost described it as magnitude 14.3 and RA 12 42 at 36.0, Dec +11 44 22. IC 3686 has an estimated diameter of 270,000 light-years making it larger compared to the Milky Way. and is classified as LINER-type active galactic nucleus galaxy according to SIMBAD. Despite listed in the Virgo Cluster catalogue as VCC 1927, it is not a member of the Virgo Cluster but a background galaxy.

<span class="mw-page-title-main">IC 3505</span> Galaxy in the constellation Coma Berenices

IC 3505 is a barred spiral galaxy located 640 million light-years away from the Solar System in the Coma Berenices constellation. With an apparent size of 0.95 by 0.35 arcmin, IC 3505 has an estimated diameter of 170,000 light-years, making it slightly larger compared to the Milky Way. It is categorized as a LINER galaxy with an active galactic nucleus emitting weak emission-lines.

<span class="mw-page-title-main">NGC 5008</span> Galaxy in the constellation Boötes

NGC 5008 is a massive barred spiral galaxy located in the Boötes constellation.

<span class="mw-page-title-main">NGC 6261</span> Galaxy in the constellation Hercules

NGC 6261 is a lenticular galaxy in the constellation of Hercules. It is located 470 million light-years away from the Solar System and has an approximate diameter of 200,000 light-years.

<span class="mw-page-title-main">IC 2431</span> Interacting galaxies in the constellation Cancer

IC 2431 are a group of interacting galaxies in the constellation of Cancer. They are located 684 million light-years away from the Solar System and were discovered on February 24, 1896, by Stephane Javelle.

<span class="mw-page-title-main">IC 1166</span> Pair of galaxies in Corona Borealis

IC 1166 are a pair of galaxies in the Corona Borealis constellation comprising IC 1166 NED01 and IC 1166 NED02. They are located 977 million light-years from the Solar System and were discovered on July 28, 1892, by Stephane Javelle.

<span class="mw-page-title-main">IC 1182</span>

IC 1182 is a type S0-a lenticular galaxy located in Hercules. It is located 464 million light-years away from the Solar System and was discovered on August 11, 1892, by Stephane Javelle. IC 1198 is a member of the Hercules Cluster, which is a part of the CfA 2 Great Wall.

<span class="mw-page-title-main">IC 1185</span> Spiral galaxy located in Hercules

IC 1185 is a type Sab spiral galaxy located in Hercules. It is located 420 million light-years from the Solar System and has an approximate diameter of 115,000 light-years. IC 1185 was discovered on June 8, 1888, by astronomer Guillaume Bigourdan and is a member of the Hercules Cluster. IC 1185 has a surface brightness of magnitude 22.7 and presents a double nucleus, which might represent a late stage of galaxy merger.

<span class="mw-page-title-main">NGC 3750</span>

NGC 3750 is a lenticular galaxy with a bar located in the constellation of Leo. It is located 450 million light-years from the Solar System and was discovered by Ralph Copeland on February 9, 1874.

<span class="mw-page-title-main">NGC 3754</span>

NGC 3754 is a small barred spiral galaxy located in Leo. It is located 447 million light-years away from the Solar System and was discovered on April 5, 1874, by Ralph Copeland.

<span class="mw-page-title-main">IC 1189</span>

IC 1189 is a S0-a lenticular galaxy with a ring structure located in Hercules. It is located 557 million light-years away from the Solar System and has an approximate diameter of 145,000 light-years. IC 1189 was discovered on June 7, 1888, by Lewis Swift. It is a member of the Hercules Cluster.

<span class="mw-page-title-main">NGC 3978</span>

NGC 3978 is a large intermediate spiral galaxy with a bar located in the constellation of Ursa Major. It is located 460 million light-years away from the Solar System and was discovered by William Herschel on March 19, 1790, but also observed by John Herschel on April 14, 1831.

<span class="mw-page-title-main">IC 3622</span> Galaxy

IC 3622 also known as PGC 3793395, is a large barred spiral galaxy located in constellation Coma Berenices. It is located 980 million light-years from the Solar System and has a diameter of 175,000 light-years. IC 3622 was discovered by Royal Harwood Frost on May 7, 1904.

<span class="mw-page-title-main">IC 3222</span>

IC 3222 known as PGC 40065 and UGC 7437, is a barred spiral galaxy with a ring structure located in the constellation of Coma Berenices. It is located 869 million light-years from the Solar System and has dimensions of 0.90 x 0.6 arcmin, meaning IC 3222 is 235,000 light-years across in diameter. This makes it a large galaxy. IC 3222 was discovered by Max Wolf on March 23, 1903.

<span class="mw-page-title-main">IC 3078</span> Galaxy located in Virgo

IC 3078 is a spiral galaxy with a ring structure located in Virgo. Its redshift is 0.066148, meaning IC 3078 is located 905 million light-years from Earth. With an apparent dimension of 0.50 x 0.5 arcmin, IC 3038 is about 133,000 light-years across. It was discovered by Royal Harwood Frost on May 7, 1904 and is listed in the Virgo Cluster catalogue as VCC 174. However, it is not a member of the Virgo Cluster, but instead a background galaxy.

References

  1. 1 2 3 "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-05-02.
  2. ↑ "HyperLeda -object description". atlas.obs-hp.fr. Retrieved 2024-05-02.
  3. ↑ Astronomy, Go. "IC 1192 | galaxy in Hercules | IC List | GO ASTRONOMY". Go-Astronomy.com. Retrieved 2024-05-02.
  4. ↑ "IC 1192". spider.seds.org. Retrieved 2024-05-02.
  5. ↑ "Index Catalog Objects: IC 1150 - 1199". cseligman.com. Retrieved 2024-05-02.
  6. ↑ Bakich, Michael E. (2024-01-01). "The Hercules galaxy cluster". Astronomy Magazine. Retrieved 2024-05-02.
  7. ↑ "Hercules Cluster of Galaxies". pages.astronomy.ua.edu. Retrieved 2024-05-02.
  8. ↑ "IC 1192 - LINER-type Active Galaxy Nucleus". simbad.u-strasbg.fr. Retrieved 2024-05-02.
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.