NGC 4618

In this article we are going to explore in depth the topic of NGC 4618, a topic that has captured the attention of millions of people around the world. From its historical relevance to its impact on modern society, NGC 4618 has been the subject of debates and discussions in different areas. Throughout these pages, we will analyze its origins, evolution and its influence on various aspects of daily life. From his manifestations in popular culture to his involvement in political and social issues, NGC 4618 has left an indelible mark that deserves to be explored in detail. In addition, we will address the different perspectives and opinions about NGC 4618, in order to offer a comprehensive and complete vision of this phenomenon.

NGC 4618
Barred spiral galaxy NGC 4618 imaged by the Hubble Space Telescope
Observation data (J2000 epoch)
ConstellationCanes Venatici[1]
Right ascension12h 41m 32.8s[2]
Declination+41° 09′ 03″[2]
Redshift544 ± 1 km/s[2]
Apparent magnitude (V)11.2[2]
Characteristics
TypeSB(rs)m[2]
Apparent size (V)4'.2 × 3'.4[2]
Notable featuresasymmetric; single spiral arm[3]
Other designations
IC 3667,[2] UGC 7853,[2] PGC 042575,[2] Arp 23,[2] VV 73[2]

NGC 4618 is a distorted barred dwarf galaxy in the constellation Canes Venatici. The galaxy is formally classified as a Sm galaxy, which means that its structure vaguely resembles the structure of spiral galaxies. The galaxy is sometimes referred to as a Magellanic spiral because of its resemblance to the Magellanic clouds.

One supernova has been observed in NGC 4618: SN 1985F (type Ib) was discovered by Alex Filippenko and Wallace L. W. Sargent on 28 February 1985.[4][5]

Structure

Unlike most spiral galaxies, NGC 4618 has a single spiral arm, which gives the galaxy an asymmetric appearance.[3] This galaxy was included in the Atlas of Peculiar Galaxies as one of three examples of nearby galaxies with single spiral arms.[6] Although NGC 4618 is labeled as peculiar, many similar galaxies have been identified.

It has been hypothesized that this galaxy's asymmetric structure may be the result of a gravitational interaction with NGC 4625.[3] Such asymmetric structure is commonly seen among many interacting galaxies. However, observations of neutral hydrogen gas in NGC 4618 and NGC 4625 imply that only some of the gas outside the optical disks of NGC 4618 is affected by the gravitational interaction.[7] This may indicate that NGC 4618's one-arm shape forms as the result of processes that are intrinsic to the galaxy itself.

Environment

As mentioned above, NGC 4618 is interacting with NGC 4625.[3]

See also

References

  1. ^ R. W. Sinnott, ed. (1988). The Complete New General Catalogue and Index Catalogue of Nebulae and Star Clusters by J. L. E. Dreyer. Sky Publishing Corporation and Cambridge University Press. ISBN 978-0-933346-51-2.
  2. ^ a b c d e f g h i j k "NASA/IPAC Extragalactic Database". Results for NGC 4618. Retrieved 2006-11-15.
  3. ^ a b c d A. Sandage; J. Bedke (1994). Carnegie Atlas of Galaxies. Washington, D.C.: Carnegie Institution of Washington. ISBN 978-0-87279-667-6.
  4. ^ Filippenko, A. V.; Sargent, W. L. W. (1985). "Unusual Object in NGC 4618". International Astronomical Union Circular (4042): 1. Bibcode:1985IAUC.4042....1F.
  5. ^ "SN 1985F". Transient Name Server. IAU. Retrieved 5 December 2024.
  6. ^ H. Arp (1966). "Atlas of Peculiar Galaxies". Astrophysical Journal Supplement. 14: 1–20. Bibcode:1966ApJS...14....1A. doi:10.1086/190147.
  7. ^ S. J. Bush; E. M. Wilcots (2004). "Neutral Hydrogen in the Interacting Magellanic Spirals NGC 4618 and NGC 4625". Astrophysical Journal. 128 (6): 2789–2796. arXiv:astro-ph/0409209. Bibcode:2004AJ....128.2789B. doi:10.1086/425876. S2CID 14636586.
  • Media related to NGC 4618 at Wikimedia Commons