NGC 855

Last updated

NGC 855
NGC855 - SDSS DR14.jpg
Observation data (J2000 epoch)
Constellation Triangulum [1]
Right ascension 02h 14m 03.4946s [1]
Declination 27° 52 37.966 [1]
Redshift 0.001975±0.000017 [1]
Heliocentric radial velocity 592 ± 5 km/s [1]
Apparent magnitude  (V)12.6 [1]
Apparent magnitude  (B)13.3 [1]
Other designations
NGC 855 • UGC 1718 • PGC 8557 • CGCG 504-035 • MCG +05-06-016 • IRAS 02111+2738 • KUG 0211+276 • 2MASX J02140361+2752378 • CN 26 613

NGC 855 is a star-forming dwarf elliptical galaxy located in the Triangulum constellation. [2] The discovery and a first description (as H 26 613) [3] was realized by William Herschel on 26 October 1786 and the findings made public through his Catalogue of Nebulae and Clusters of Stars, published the same year. [4]

Contents

NGC 855's relative velocity to the cosmic microwave background is 343 ± 18 km/s (343 ± 18) km/s, corresponding to a Hubble distance of 5.06 ± 0.44 Mpc (~16.5 million ly). [1] There is some uncertainty about its precise distance since two surface brightness fluctuation measurements give a distance of 9.280 ± 0.636 Mpc (~30.3 million ly), a range outside the Hubble distance determined by the galaxy's redshift survey. [5]

Star formation

Using infrared data collected from two regions in the center of the galaxy by the Spitzer Space Telescope, astronomers were able to suggest NGC 855 to be a star-forming galaxy. [2] Its HI distribution (Neutral atomic hydrogen emission lines) suggests the star-forming activity might have been triggered by a minor merger. [2]

See also

Related Research Articles

<span class="mw-page-title-main">NGC 3982</span> Galaxy in the constellation Ursa Major

NGC 3982(also known as UGC 6918) is an intermediate spiral galaxy approximately 68 million light-years away in the constellation Ursa Major. It was discovered by William Herschel on April 14, 1789, and misclassified as a planetary nebula. NGC 3982 is a part of the M109 Group.

<span class="mw-page-title-main">NGC 4873</span> Galaxy in the constellation Coma Berenices

NGC 4873 is a lenticular galaxy located about 270 million light-years away in the constellation of Coma Berenices. NGC 4873 was discovered by astronomer Heinrich d'Arrest on May 10, 1863. The galaxy is a member of the Coma Cluster.

<span class="mw-page-title-main">NGC 6061</span> Galaxy in the constellation Hercules

NGC 6061 is a lenticular galaxy with radio activity located about 490 million light-years away in the constellation Hercules. The galaxy is classified as a head-tail radio galaxy and was discovered by astronomer Lewis Swift on June 8, 1886. NGC 6061 is a member of the Hercules Cluster.

<span class="mw-page-title-main">NGC 4694</span> Lenticular galaxy in the constellation Virgo

NGC 4694 is a lenticular galaxy in the constellation Virgo. Its velocity with respect to the cosmic microwave background is 1481 ± 23 km/s, which corresponds to a Hubble distance of 71.3 ± 5.1 Mly (21.85 ± 1.57 Mpc). However, six non redshift measurements give a distance of 28.51 ± 7.23 Mly (8.742 ± 2.218 Mpc). The galaxy was discovered by William Herschel on March 15, 1784.

<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 5486</span> Galaxy in the constellation Ursa Major

NGC 5486 is an irregular galaxy in the constellation Ursa Major 110 million light-years from Earth.

<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 2008</span> Spiral galaxy in the constellation Pictor

NGC 2008 is a distant spiral galaxy located in the constellation Pictor. Its speed relative to the cosmic microwave background is 10,367 ± 11 km/s, which corresponds to a Hubble distance of 153 ± 11 Mpc. NGC 2008 was discovered by British astronomer John Herschel in 1834. The luminosity class of NGC 2008 is III with an apparent magnitude of 13.2.

<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 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 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 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 1340</span> Elliptical galaxy in the constellation Fornax

NGC 1340 is an elliptical galaxy located in the constellation Fornax. Its speed relative to the cosmic microwave background is 1,126 ± 17 km/s, which corresponds to a Hubble Distance of 16.6 ± 1.2 Mpc. It was discovered by the German-British astronomer William Herschel in 1790, but it was added to the New General Catalog under the designation NGC 1344 later.

<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 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 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.

References

  1. 1 2 3 4 5 6 7 8 "By Name | NASA/IPAC Extragalactic Database". ned.ipac.caltech.edu. Retrieved 5 November 2023.
  2. 1 2 3 Li, Sheng-Peng; Gu, Qiu-Sheng; Zhao, Ying-He; Huang, Jia-Sheng; Luo, Xin-Lian (2007). "A Study of the Star-forming Dwarf Galaxy NGC 855 with Spitzer". Chinese Journal of Astronomy and Astrophysics . 7 (6): 764. Bibcode:2007ChJAA...7..764L. doi: 10.1088/1009-9271/7/6/03 . ISSN   1009-9271.
  3. "Catalogue of Nebulae and Clusters of Stars".
  4. "Herschel Catalog". www.messier.seds.org. Retrieved 6 November 2023.
  5. "NED Query Results for NGC 855". ned.ipac.caltech.edu. Retrieved 6 November 2023.