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- Q942362 subject Q7215864.
- Q942362 abstract "GCl 38 is a globular cluster located in theconstellation Hercules.It was discovered in 1958 by Sidney van den Bergh and Halton Arp during inspection of the photographic plates from the Palomar Sky Survey.This is a round, diffuse cluster located in the outerhalo of the Milky Way galaxy. It is about 3–4 billion years younger than a typical galactic cluster.The metallicity of the cluster is [Fe/H] = −1.50, indicating a lower abundance of elements with mass greater that helium compared to the Sun. The combined mass of the main sequence stars in the cluster is 1340 ± 50 solar masses, and the combined mass of observed stars within the half-light radius is 6020 ± 50 solar masses. (This is the inner radius of the cluster that emits half the total luminosity.) These mass estimates provide lower bounds for determining the total mass of the cluster. The median radial velocity of stars within the cluster is 72.19 ± 0.18 km/s.Because of the cluster's location on the outer fringes of the Milky Way, it was used as a test case for modified newtonian dynamics (MOND). This is an alternative hypothesis to explain the galactic rotation problem.".
- Q942362 wikiPageWikiLink Q10448.
- Q942362 wikiPageWikiLink Q11276.
- Q942362 wikiPageWikiLink Q12129.
- Q942362 wikiPageWikiLink Q1354016.
- Q942362 wikiPageWikiLink Q1475614.
- Q942362 wikiPageWikiLink Q1503556.
- Q942362 wikiPageWikiLink Q180892.
- Q942362 wikiPageWikiLink Q2703.
- Q942362 wikiPageWikiLink Q321.
- Q942362 wikiPageWikiLink Q3450.
- Q942362 wikiPageWikiLink Q453729.
- Q942362 wikiPageWikiLink Q523.
- Q942362 wikiPageWikiLink Q525.
- Q942362 wikiPageWikiLink Q531.
- Q942362 wikiPageWikiLink Q560.
- Q942362 wikiPageWikiLink Q577.
- Q942362 wikiPageWikiLink Q7215864.
- Q942362 wikiPageWikiLink Q8928.
- Q942362 comment "GCl 38 is a globular cluster located in theconstellation Hercules.It was discovered in 1958 by Sidney van den Bergh and Halton Arp during inspection of the photographic plates from the Palomar Sky Survey.This is a round, diffuse cluster located in the outerhalo of the Milky Way galaxy. It is about 3–4 billion years younger than a typical galactic cluster.The metallicity of the cluster is [Fe/H] = −1.50, indicating a lower abundance of elements with mass greater that helium compared to the Sun.".
- Q942362 label "GCl 38".