NGC 925
Ang NGC 925 ay isang galaksiyang espayral na may bara, na matatagpuan sa 30 milyong taong-liwanag ang layo sa konstelasyon ng Triangulum. Ang klasipikasyong morpolohikal na ito sa kalawakan ay SB(s)d.[1][2][3][4][5][6][7][8]
Mga sanggunian
[baguhin | baguhin ang wikitext]- ↑ "NASA/IPAC Extragalactic Database". Results for NGC 925. Nakuha noong 2008-12-28.
- ↑ Buta, Ronald J.; atbp. (2007), Atlas of Galaxies, Cambridge University Press, pp. 13–17, ISBN 0521820480.
- ↑ Pisano, D. J.; atbp. (June 2007), "An H I Survey of Six Local Group Analogs. I. Survey Description and the Search for High-Velocity Clouds", The Astrophysical Journal, 662 (2): 959–968, arXiv:astro-ph/0703279, Bibcode:2007ApJ...662..959P, doi:10.1086/517986.
- ↑ Tully, R. B. (April 1980), "Nearby groups of galaxies. I - The NGC 1023 group", Astrophysical Journal, Part 1, 237: 390–403, Bibcode:1980ApJ...237..390T, doi:10.1086/157881.
- ↑ Pisano, D. J.; Wilcots, Eric M.; Elmegreen, Bruce G. (August 2000), "Structure and Star Formation in NGC 925", The Astronomical Journal, 120 (2): 763–776, arXiv:astro-ph/0004219, Bibcode:2000AJ....120..763P, doi:10.1086/301464.
- ↑ Silbermann, N. A.; atbp. (October 1996), "The Hubble Space Telescope Key Project on the Extragalactic Distance Scale. VI. The Cepheids in NGC 925", Astrophysical Journal, 470: 1, Bibcode:1996ApJ...470....1S, doi:10.1086/177845.
{{citation}}: CS1 maint: multiple names: authors list (link) - ↑ Martin, Pierre; Roy, Jean-Rene (April 1994), "The influence of bars on the chemical composition of spiral galaxies", Astrophysical Journal, Part 1, 424 (2): 599–614, Bibcode:1994ApJ...424..599M, doi:10.1086/173917.
- ↑ Skrutskie, M. F.; atbp. (February 2006), "The Two Micron All Sky Survey (2MASS)", The Astronomical Journal, 131 (2): 1163–1183, Bibcode:2006AJ....131.1163S, doi:10.1086/498708.
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