10 Hygiea (Galician Wikipedia)

Analysis of information sources in references of the Wikipedia article "10 Hygiea" in Galician language version.

refsWebsite

Global rank Galician rank

6doi.org

2^nd place

7^th place

5web.archive.org

1^st place

3nasa.gov

75^th place

47^th place

2harvard.edu

18^th place

38^th place

1webcitation.org

24^th place

63^rd place

1earthlink.net

7,693^rd place

9,028^th place

1springerlink.com

2,569^th place

747^th place

1helsinki.fi

1,670^th place

439^th place

1unipi.it

low place

7,036^th place

1cas.cz

2,066^th place

7,138^th place

1nih.gov

4^th place

6^th place

1archive.org

6^th place

8^th place

1jas.org.jo

low place

1allaboutastro.com

low place

1usra.edu

2,838^th place

1,645^th place

1gaoran.ru

low place

allaboutastro.com

Ballauer Observatory, ed. (2004). "What Can I See Through My Scope?". Arquivado dende o orixinal o 22-06-2013. Consultado o 20-07-2008.

archive.org

John Russell Hind (1852). G. P. Putnam, ed. The Solar System: Descriptive Treatise Upon the Sun, Moon, and Planets, Including an Account of All the Recent Discoveries. p. 126.

cas.cz

astro.cas.cz

O. Gingerich (2006). "The Path to Defining Planets" (PDF). Harvard-Smithsonian Center for Astrophysics and IAU EC Planet Definition Committee chair. Consultado o 13-03-2007.

doi.org

dx.doi.org

Baer, James; Chesley, Steven R. (2008). "Astrometric masses of 21 asteroids, and an integrated asteroid ephemeris" (PDF). Celestial Mechanics and Dynamical Astronomy (Springer Science+Business Media B.V. 2007) 100 (2008): 27–42. doi:10.1007/s10569-007-9103-8. Arquivado dende o orixinal (PDF) o 24-02-2011. Consultado o 11-11-2008.
M. Kaasalainen (2002). "Models of Twenty Asteroids from Photometric Data" (PDF). Icarus 159: 369. doi:10.1006/icar.2002.6907. Arquivado dende o orixinal (PDF) o 16-02-2008. Consultado o 23-06-2009.
L.F. Lim; McConnochie, T.; Belliii, J.; Hayward, T. (2005). "Thermal infrared (8–13 µm) spectra of 29 asteroids: the Cornell Mid-Infrared Asteroid Spectroscopy (MIDAS) Survey". Icarus 173: 385. doi:10.1016/j.icarus.2004.08.005.
A. O. Leuschner (15-07-1922). National Academy of Sciences, ed. "Comparison of Theory with Observation for the Minor planets 10 Hygiea and 175 Andromache with Respect to Perturbations by Jupiter". Proceedings of the National Academy of Sciences of the United States of America 8 (7): 170–173. PMC 1085085. PMID 16586868. doi:10.1073/pnas.8.7.170.
Barucci, M (2002). "10 Hygiea: ISO Infrared Observations". Icarus 156: 202. doi:10.1006/icar.2001.6775.
A. Storrs (1999). "Imaging Observations of Asteroids with Hubble Space Telescope". Icarus 137: 260. doi:10.1006/icar.1999.6047.

earthlink.net

home.earthlink.net

Jim Baer (2008). Personal Website, ed. "Recent Asteroid Mass Determinations". Arquivado dende o orixinal o 08-07-2013. Consultado o 03-12-2008.

gaoran.ru

L’vov V.N., Smekhacheva R.I., Smirnov S.S., Tsekmejster S.D. Central (Pulkovo) Astronomical Observatory of Russian Academy of Sciences, ed. "Some Peculiarities in the Hildas' Motion" (PDF). Consultado o 06-05-2020.

harvard.edu

cfa.harvard.edu

Minor Planet Center (ed.). "Bright Minor Planets 2000". Consultado o 21-05-2008. ^{[Ligazón morta]}

adsabs.harvard.edu

Hartnup, J. (1850). "Observations of Hygeia". Monthly Notices of the Royal Astronomical Society 10: 162.

helsinki.fi

rni.helsinki.fi

M. Kaasalainen (2002). "Models of Twenty Asteroids from Photometric Data" (PDF). Icarus 159: 369. doi:10.1006/icar.2002.6907. Arquivado dende o orixinal (PDF) o 16-02-2008. Consultado o 23-06-2009.

jas.org.jo

Moh'd Odeh. "The Brightest Asteroids". The Jordanian Astronomical Society. Arquivado dende o orixinal o 13-08-2007. Consultado o 21-05-2008.

nasa.gov

ssd.jpl.nasa.gov

"JPL Small-Body Database Browser: 10 Hygiea". Consultado o 07-09-2008.
"JPL Close-Approach Data: 10 Hygiea". 27-11-2009 últimas observacións. Consultado o 02-03-2010.

iau-comm4.jpl.nasa.gov

"Masa de Hygiea" 0,445 / "Masa do cinto" Arquivado 31 de outubro de 2008 en Wayback Machine. 15 = 0,0296

nih.gov

ncbi.nlm.nih.gov

A. O. Leuschner (15-07-1922). National Academy of Sciences, ed. "Comparison of Theory with Observation for the Minor planets 10 Hygiea and 175 Andromache with Respect to Perturbations by Jupiter". Proceedings of the National Academy of Sciences of the United States of America 8 (7): 170–173. PMC 1085085. PMID 16586868. doi:10.1073/pnas.8.7.170.

springerlink.com

Baer, James; Chesley, Steven R. (2008). "Astrometric masses of 21 asteroids, and an integrated asteroid ephemeris" (PDF). Celestial Mechanics and Dynamical Astronomy (Springer Science+Business Media B.V. 2007) 100 (2008): 27–42. doi:10.1007/s10569-007-9103-8. Arquivado dende o orixinal (PDF) o 24-02-2011. Consultado o 11-11-2008.

unipi.it

hamilton.dm.unipi.it

Department of Mathematics, University of Pisa, Italy (ed.). "AstDys (10) Hygiea Ephemerides". Consultado o 26-06-2010.

usra.edu

lpi.usra.edu

James L. Hilton. Lunar and Planetar Institute, ed. "Asteroid Masses and Densities" (PDF). U.S. Naval Observatory. Consultado o 26-08-2008.

web.archive.org

Baer, James; Chesley, Steven R. (2008). "Astrometric masses of 21 asteroids, and an integrated asteroid ephemeris" (PDF). Celestial Mechanics and Dynamical Astronomy (Springer Science+Business Media B.V. 2007) 100 (2008): 27–42. doi:10.1007/s10569-007-9103-8. Arquivado dende o orixinal (PDF) o 24-02-2011. Consultado o 11-11-2008.
M. Kaasalainen (2002). "Models of Twenty Asteroids from Photometric Data" (PDF). Icarus 159: 369. doi:10.1006/icar.2002.6907. Arquivado dende o orixinal (PDF) o 16-02-2008. Consultado o 23-06-2009.
"Masa de Hygiea" 0,445 / "Masa do cinto" Arquivado 31 de outubro de 2008 en Wayback Machine. 15 = 0,0296
Moh'd Odeh. "The Brightest Asteroids". The Jordanian Astronomical Society. Arquivado dende o orixinal o 13-08-2007. Consultado o 21-05-2008.
Ballauer Observatory, ed. (2004). "What Can I See Through My Scope?". Arquivado dende o orixinal o 22-06-2013. Consultado o 20-07-2008.

webcitation.org

Jim Baer (2008). Personal Website, ed. "Recent Asteroid Mass Determinations". Arquivado dende o orixinal o 08-07-2013. Consultado o 03-12-2008.