IC 3275

Last updated
IC 3275
IC3275 - SDSS DR14.jpg
IC 3275 taken by SDSS
Observation data
Constellation Virgo
Right ascension 12h 24m 19.477s
Declination +10d 26m 46.80s
Redshift 0.060127
Heliocentric radial velocity 18,026 km/s
Distance 811 Mly (248.6 Mpc)
Apparent magnitude  (V)16.1
Characteristics
Type S, Sbc, Sc
Size120,000 ly
Apparent size  (V)0.55 x 0.33 arcmin
Other designations
PGC 165137, 2MASX J12241948+1026468, SDSS J122419.47+102646.7, ASK 275598.0, MAPS-NGP O_496_0134146, [DCY96] 132, VPC 0341, SPIDER J186.08115+10.44633, GALEXASC J122419.60+102647.2, 2MASS J12241948+1026467, LEDA 165137

IC 3275 is a spiral galaxy with a ring structure [1] located in the Virgo constellation. [2] [3] [4] It is located 811 million light-years away from the Solar System and has an approximate diameter of 120,000 light-years across. [5] IC 3275 was discovered on May 7, 1904, by Royal Harwood Frost. [6]

Supernova

One supernova has been discovered in IC 3275 so far: SN 2024fid.

SN 2024fid

SN 2024fid was discovered by the ATLAS program (Asteroid Terrestrial-impact Last Alert System) [7] on March 29, 2024. [8] The supernova was reported by J. Tonry, L. Denneau, H. Weiland, A. Lawrence and R. Siverd from University of Hawaii, N. Erasmus, W. Koorts from South African Astronomical Observatory, A. Jordan, V. Suc from UAI, Obstech and other astronomers. They saw it via unfiltered images from orange-ATLAS which was taken using an ATLAS telescope at Mauna Loa. [8] SN 2024fid was located at right ascension (12h 24m 18s.866) and declination (+10 degrees 26' 46" 40), with a magnitude of 18.8. [9] The supernova was Type Ia-91bg-like. [10]

Related Research Articles

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<span class="mw-page-title-main">NGC 3336</span> Galaxy in the constellation Hydra

NGC 3336 is a barred spiral galaxy located about 190 million light-years away in the constellation Hydra. It was discovered by astronomer John Herschel on March 24, 1835. NGC 3336 is a member of the Hydra Cluster.

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<span class="mw-page-title-main">NGC 1268</span> Spiral galaxy in the constellation Perseus

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<span class="mw-page-title-main">NGC 1282</span> Galaxy in the constellation Perseus

NGC 1282 is an elliptical galaxy located about 230 million light-years away in the constellation Perseus. It was discovered by astronomer Guillaume Bigourdan on October 23, 1884. NGC 1282 is a member of the Perseus Cluster.

<span class="mw-page-title-main">NGC 694</span> Spiral galaxy in the constellation Aries

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<span class="mw-page-title-main">NGC 819</span> Galaxy in the constellation Triangulum

NGC 819 is a spiral galaxy approximately 302 million light-years away from Earth in the constellation of Triangulum. It forms a visual pair with the galaxy NGC 816 5.7' WNW.

<span class="mw-page-title-main">NGC 4316</span> Spiral galaxy in the constellation Virgo

NGC 4316 is an edge-on spiral galaxy located about 70 million light-years away in the constellation Virgo. It was discovered by astronomer Wilhelm Tempel on March 17, 1882. NGC 4316 is a member of the Virgo Cluster and is classified as LINER and as a Seyfert 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 6261</span> Galaxy in the constellation Hercules

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<span class="mw-page-title-main">IC 4040</span> Galaxy in the constellation Coma Berenices

IC 4040 is a type SABc spiral galaxy with a bar in Coma Berenices. It is located 353 million light-years away from the Solar System and has an estimated diameter of 105,000 light-years making it slightly larger than the Milky Way. IC 4040 was discovered on April 12, 1891, by Guillaume Bigourdan and is a member of the Coma Cluster.

<span class="mw-page-title-main">NGC 3746</span>

NGC 3746 is a large barred spiral galaxy with a ring structure located in the Leo constellation. It is located 449 million light-years from the Solar System and has an approximate diameter of 165,000 light-years. NGC 3746 was discovered by Ralph Copeland on 9 February 1874 with subsequent observations made by Hermann Kobold, Lawrence Parsons and John Louis Emil Dreyer.

<span class="mw-page-title-main">IC 2759</span> Elliptical galaxy in the constellation of Leo

IC 2759 is a small type E elliptical galaxy located in the constellation of Leo. It is located 350 million light-years away from the Solar System and was discovered on April 24, 1897, by Guillaume Bigourdan. Sometimes IC 2759 is confused with the spiral galaxy, PGC 34882 which is located south of the galaxy.

<span class="mw-page-title-main">IC 5145</span>

IC 5145 is a type Sab spiral galaxy located in the constellation Pegasus. It is located 356 million light-years from the Solar System and was discovered by Edward Emerson Barnard, although the year he discovered it is unknown.

<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">NGC 7222</span> Large barred spiral galaxy with a ring structure

NGC 7222 is a large barred spiral galaxy with a ring structure, located in the constellation Aquarius. It is located 570 million light-years away from the Solar System and was discovered by German astronomer, Albert Marth on August 11, 1864.

<span class="mw-page-title-main">IC 2498</span>

IC 2498 known as PGC 27668, is a type Sb barred spiral galaxy located in constellation Leo. It is located 469 million light-years away from the Solar System and was discovered by Stephane Javelle on April 30, 1896.

<span class="mw-page-title-main">UGC 9684</span> Galaxy located in Boötes

UGC 9684 is a barred spiral galaxy with a ring structure in the Boötes constellation. It is located 250 million light-years from the Solar System and has an approximate diameter of 90,000 light-years.

<span class="mw-page-title-main">IC 1050</span>

IC 1050 is a type Sbc spiral galaxy located in constellation Boötes. It is located 491 million light-years from the Solar System and has an approximate diameter of 130,000 light-years. IC 1050 was discovered by Stephane Javelle on June 3, 1892.

<span class="mw-page-title-main">IC 4588</span>

IC 4588 is a type E elliptical galaxy located in the constellation Serpens. It is located 729 million light-years from the Solar System and has a dimension of 0.30 x 0.3 arcmin meaning its diameter is 64,000 light-years across. IC 4588 was discovered by Stephane Javelle on July 15, 1903.

References

  1. ↑ "HyperLeda -object description". atlas.obs-hp.fr. Retrieved 2024-05-06.
  2. ↑ "Revised IC Data for IC 3275". spider.seds.org. Retrieved 2024-05-06.
  3. ↑ Astronomy, Go. "IC 3275 | galaxy in Virgo | IC List | GO ASTRONOMY". Go-Astronomy.com. Retrieved 2024-05-06.
  4. ↑ Ford, Dominic. "IC3275 (Galaxy)". In-The-Sky.org. Retrieved 2024-05-06.
  5. ↑ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-05-06.
  6. ↑ "Index Catalog Objects: IC 3250 - 3299". cseligman.com. Retrieved 2024-05-06.
  7. ↑ "ATLAS - The ATLAS Project". atlas.fallingstar.com. Retrieved 2024-05-06.
  8. 1 2 "Discovery certificate for object 2024fid | Transient Name Server". www.wis-tns.org. Retrieved 2024-05-06.
  9. ↑ "Latest Supernovae". www.rochesterastronomy.org. Retrieved 2024-05-06.
  10. ↑ "SN 2024fid | Transient Name Server". www.wis-tns.org. Retrieved 2024-05-06.
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