NGC 411

In today's world, NGC 411 is a topic of constant debate and controversy. Whether it's politics, technology, culture or society, NGC 411 has captured the attention of people of all ages and backgrounds. In this article, we will explore different facets related to NGC 411 and analyze its impact on our lives. From the latest scientific advances to the opinions of experts in the field, we will seek to shed light on the topic and provide a complete and enriching overview for our readers. Through interviews, research, and concrete examples, we hope to shed light on NGC 411 and help our readers better understand its relevance in today's world.
NGC 411
Hubble Space Telescope image of the open cluster NGC 411
Credit: NASA/ESA
Observation data (J2000 epoch)
Right ascension01h 07m 55.95s[1]
Declination−71° 46′ 04.5″[1]
Distance179,000 ± 13,000 ly (55,000 ± 4,000 pc)[2]
Apparent magnitude (V)12.1[1]
Apparent dimensions (V)2.1′ × 1.9′[1]
Physical characteristics
Mass3.0×104[3] M☉
Estimated age1.5 billion years[4]
Other designationsKron 60, Lindsay 82, ESO 51-19[1]
Associations
ConstellationTucana
See also: Open cluster, List of open clusters

NGC 411 is a globular cluster located approximately 55,000 pc (180,000 ly) from Earth in the constellation Tucana. It was discovered in 1826 by James Dunlop. It was described by Dreyer as "extremely faint, pretty large, round, gradually very little brighter middle".[5] At a distance of about 180,000 light years (55,000 parsecs), it is located within the Small Magellanic Cloud.[2] It has a mass of about 3.0×104 M☉, and a luminosity of about 8.0×104 L☉.[3]

NGC 411 was imaged by the Hubble Space Telescope in 2013, showing an abundance of stars ranging from blue to red.[6] In particular, this seemed to suggest that the cluster was much younger than previously thought: its age has been estimated at 1.5 billion years old, relatively young in astronomical terms.[4][6] However, these results have been challenged by another group who state that these young stars may actually just be background stars, and are thus physically unrelated.[7]

See also

References

  1. ^ a b c d e "NGC 411". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 6 February 2017.
  2. ^ a b "NASA/IPAC Extragalactic Database". Results for NGC 0411. Retrieved 2 September 2016.
  3. ^ a b Song, Ying-Yi; Mateo, Mario; Bailey, John I.; Walker, Matthew G.; Roederer, Ian U.; Olszewski, Edward W.; Reiter, Megan; Kremin, Anthony (2021). "Dynamical masses and mass-to-light ratios of resolved massive star clusters – II. Results for 26 star clusters in the Magellanic Clouds". Monthly Notices of the Royal Astronomical Society. 504 (3): 4160–4191. arXiv:2104.06882. doi:10.1093/mnras/stab1065.
  4. ^ a b Li, C.; de Grijs, R.; Bastian, N.; Deng, L.; Niederhofer, F.; Zhang, C. (2016). "The tight subgiant branch of the intermediate-age star cluster NGC 411 implies a single-aged stellar population". Monthly Notices of the Royal Astronomical Society. 461 (3): 3212–3221. arXiv:1606.05394. Bibcode:2016MNRAS.461.3212L. doi:10.1093/mnras/stw1491.
  5. ^ "New General Catalog Objects: NGC 400 - 449". Cseligman. Retrieved 6 February 2017.
  6. ^ a b "Hubble Finds Appearances can be Deceptive". www.nasa.gov. 2013.
  7. ^ Cabrera-Ziri, I.; et al. (2016). "No evidence for younger stellar generations within the intermediate-age massive clusters NGC 1783, NGC 1806 and NGC 411". Monthly Notices of the Royal Astronomical Society. 459 (4): 4218–4223. arXiv:1604.06106. Bibcode:2016MNRAS.459.4218C. doi:10.1093/mnras/stw966.
  • Media related to NGC 411 at Wikimedia Commons
Stub icon

This star cluster–related article is a stub. You can help Wikipedia by expanding it.

Wikious
Boobota
Sagapedia