M105 (Italian Wikipedia)

Analysis of information sources in references of the Wikipedia article "M105" in Italian language version.

Last modified: 15:15:36, 19 September 2026 (UTC)

Ref.Un. Ref.Website

Global rank Italian rank

240^th place

249^th place

14^th place

63^rd place

2^nd place

3^rd place

1,720^th place

500^th place

adsabs.harvard.edu (Global: 14^th place; Italian: 63^rd place)

P. Fouque, E. Gourgoulhon, P. Chamaraux, G. Paturel, Groups of galaxies within 80 Mpc. II - The catalogue of groups and group members, in Astronomy and Astrophysics Supplement, vol. 93, 1992, pp. 211-233.
A. Garcia, General study of group membership. II - Determination of nearby groups, in Astronomy and Astrophysics Supplement, vol. 100, 1993, pp. 47-90.
G. Giuricin, C. Marinoni, L. Ceriani, A. Pisani, Nearby Optical Galaxies: Selection of the Sample and Identification of Groups, in Astrophysical Journal, vol. 543, 2000, pp. 178-194, DOI:10.1086/317070.

NASA/IPAC Extragalactic Database, su Results for M105. URL consultato il 16 novembre 2006.

(EN) Courtney Seligman, NGC Objects: NGC 3350 - 3399, in Celestial Atlas. URL consultato il 22 aprile 2020.

Kristen L. Shapiro, Michele Cappellari e Tim De Zeeuw, The black hole in NGC 3379: a comparison of gas and stellar dynamical mass measurements with HST and integral-field data, in Monthly Notices of the Royal Astronomical Society, vol. 370, n. 2, 1º agosto 2006, pp. 559–579, DOI:10.1111/j.1365-2966.2006.10537.x. URL consultato il 19 settembre 2026.
G. Giuricin, C. Marinoni, L. Ceriani, A. Pisani, Nearby Optical Galaxies: Selection of the Sample and Identification of Groups, in Astrophysical Journal, vol. 543, 2000, pp. 178-194, DOI:10.1086/317070.

Kristen L. Shapiro, Michele Cappellari e Tim De Zeeuw, The black hole in NGC 3379: a comparison of gas and stellar dynamical mass measurements with HST and integral-field data, in Monthly Notices of the Royal Astronomical Society, vol. 370, n. 2, 1º agosto 2006, pp. 559–579, DOI:10.1111/j.1365-2966.2006.10537.x. URL consultato il 19 settembre 2026.