NGC 3753

In this article, the topic of NGC 3753 will be addressed from different perspectives, with the purpose of exploring its implications, applications and relevance today. Its historical context, its possible impacts in various areas and its relevance in the current panorama will be analyzed in detail. Likewise, its possible future implications will be delved into and various points of view on NGC 3753 will be discussed. Through a journey through different approaches and opinions, the aim is to provide the reader with a comprehensive and detailed vision of this topic, with the aim of encouraging debate and reflection.

NGC 3753
NGC 3753 is sandwiched between NGC 3754 and NGC 3751
Observation data (J2000 epoch)
ConstellationLeo
Right ascension11h 37m 53.90s
Declination+21d 58m 53.0s
Redshift0.029064
Heliocentric radial velocity8,713 km/s
Distance435 Mly (133.37 Mpc)
Group or clusterCopeland Septet
Apparent magnitude (V)14.52
Characteristics
TypeSb, LINER, SAb
Size258,000 ly
Other designations
PGC 36016, UGC 6602, VV 282a, KUG 1135+222, MCG +04-28-010, SPRC 203, Copeland Septet NED06, HCG 057A, 2MASS J11375380+2158520, 2MASX J11375378+2158520, SDSS J113753.78+215851.8, WBL 343-005, NSA 139944, SSTL2 J113753.80+215852.4, LEDA 36016

NGC 3753 is a large barred spiral galaxy located in the Leo constellation.[1] It is located 435 million light-years away from the Solar System[2] and was discovered on February 9, 1874, by Ralph Copeland.[3]

NGC 3753 is classified as a LINER galaxy meaning, it presents an emission spectrum characterized by broad lines of weak ionized atoms. It also has a luminosity class of I-II.[2] NGC 3753 is viewed edge-on.

Copeland Septet

Sloan Digital Sky Survey image of NGC 3753 and two members of Copeland Septet.

NGC 3753 is a member of the Copeland Septet which consists of 7 galaxies discovered by Copeland in 1874.[4] The other members are NGC 3746, NGC 3745, NGC 3748, NGC 3750, NGC 3751 and NGC 3754.[5]

Halton Arp noticed the 7 galaxies in the group, in which he published the article in 1966.[6] The group is designated as Arp 320 along another galaxy, PGC 36010.[7]

This group was observed by Paul Hickson in which he included them in his article in 1982.[8] The group is known as Hickson 57 in which NGC 3753 is the dominant member.[9]

References

  1. ^ "NGC 3753 - Barred Spiral Galaxy in Leo | TheSkyLive.com". theskylive.com. Retrieved 2024-05-01.
  2. ^ a b "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-05-01.
  3. ^ "New General Catalog Objects: NGC 3750 - 3799". cseligman.com. Retrieved 2024-05-01.
  4. ^ Bakich, Michael E. (2024-01-01). "Copeland's Septet". Astronomy Magazine. Retrieved 2024-05-01.
  5. ^ "Copeland's Septet (Hickson Compact Group 57) – Constellation Guide". www.constellation-guide.com. Retrieved 2024-05-01.
  6. ^ "NED Search Results for ARP 320". ned.ipac.caltech.edu. Retrieved 2024-05-01.
  7. ^ "Copeland's Septet (Arp 320) - Astronomy Magazine - Interactive Star Charts, Planets, Meteors, Comets, Telescopes". cs.astronomy.com. Retrieved 2024-05-01.
  8. ^ Hickson, P. (1982-04-01). "Systematic properties of compact groups of galaxies". The Astrophysical Journal. 255: 382–391. Bibcode:1982ApJ...255..382H. doi:10.1086/159838. ISSN 0004-637X.
  9. ^ "N3700-N3799". astrovalleyfield.ca. Retrieved 2024-05-01.