Delta Lyrae cluster

Delta Lyrae cluster is a sparse open cluster of stars located about 1,220[2] light years away in the northern constellation of Lyra. Centered on the member star Delta2 Lyrae for which it is named,[3] it was first suspected in 1959 by American astronomer Charles B. Stephenson, then was later concluded not to exist by German astronomer Werner Bronkalla in 1963. However, subsequent photometric observations at the Palomar and Mount Wilson observatories led American astronomer Olin J. Eggen to demonstrate that there was an actual cluster, at least for the observed stars down to absolute magnitude +5.5. Eggen's study found at least 33 members.[7]

Delta Lyrae cluster
Observation data (J2000 epoch)
ConstellationLyra
Right ascension 18h 53m 30.(0)s[1]
Declination+36° 55′ 0(0)″[1]
Distance1,220 ly (373 pc)[2]
Apparent magnitude (V)3.8[3]
Apparent dimensions (V)20′[3]
Physical characteristics
Mass589[4] M☉
Estimated age49 Myr[5]
Other designationsStephenson 1[6]
Lyra with the δ Lyrae pair and surrounding cluster stars left of centre

The cluster has a visual magnitude of 3.8 and spans an angular diameter of 20 arc minutes.[3] The tidal radius of the cluster is 38 ly (11.5 pc) and it has an estimated combined mass of 589 times the mass of the Sun.[4] Based upon its estimated age and motion through space, it may be associated with the Gould Belt.[5] It includes an Algol variable star, BD+36° 3317, discovered in 2007 from Spain: this is a spectroscopic binary star system that undergoes regular eclipses because the orbital plane is nearly aligned with the line of sight to the Earth.[2]

See Also
gollark: The migration to systemd as its init system started in August 2012, and it became the default on new installations in October 2012. It replaced the SysV-style init system, used since the distribution inception. On 24 February 2020, Aaron Griffin announced that due to his limited involvement with the project, he would, after a voting period, transfer control of the project to Levente Polyak. This change also led to a new 2-year term period being added to the Project Leader position. The end of i686 support was announced in January 2017, with the February 2017 ISO being the last one including i686 and making the architecture unsupported in November 2017. Since then, the community derivative Arch Linux 32 can be used for i686 hardware.
gollark: Vinet led Arch Linux until 1 October 2007, when he stepped down due to lack of time, transferring control of the project to Aaron Griffin.
gollark: Originally only for 32-bit x86 CPUs, the first x86_64 installation ISO was released in April 2006.
gollark: Inspired by CRUX, another minimalist distribution, Judd Vinet started the Arch Linux project in March 2002. The name was chosen because Vinet liked the word's meaning of "the principal," as in "arch-enemy".
gollark: Arch Linux has comprehensive documentation, which consists of a community wiki known as the ArchWiki.

References
  1. Wu, Zhen-Yu; et al. (November 2009), "The orbits of open clusters in the Galaxy", Monthly Notices of the Royal Astronomical Society, 399 (4): 2146–2164, arXiv:0909.3737, Bibcode:2009MNRAS.399.2146W, doi:10.1111/j.1365-2966.2009.15416.x.
  2. Özdarcan, O.; et al. (July 2012), "BD+36 3317: An algol type eclipsing binary in Delta Lyrae cluster", New Astronomy, 17 (5): 483–487, arXiv:1207.0194, Bibcode:2012NewA...17..483O, doi:10.1016/j.newast.2011.12.002.
  3. Crossen, Craig; Rhemann, Gerald (2012), Sky Vistas: Astronomy for Binoculars and Richest-Field Telescopes, Springer Science & Business Media, ISBN 3709106265, retrieved 2015-11-10.
  4. Piskunov, A. E.; et al. (January 2008), "Tidal radii and masses of open clusters", Astronomy and Astrophysics, 477 (1): 165–172, Bibcode:2008A&A...477..165P, doi:10.1051/0004-6361:20078525.
  5. Piskunov, A. E.; et al. (January 2006), "Revisiting the population of Galactic open clusters", Astronomy and Astrophysics, 445 (2): 545–565, arXiv:astro-ph/0508575, Bibcode:2006A&A...445..545P, doi:10.1051/0004-6361:20053764.
  6. "NAME del Lyr Cluster". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2015-11-10.
  7. Eggen, O. J. (April 1968), "Photometric evidence for the existence of a delta Lyrae cluster", Astrophysical Journal, 152: 77, Bibcode:1968ApJ...152...77E, doi:10.1086/149525.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.