Gliese 436 Referensi
1 2 3 4 5 van Leeuwen, F. (November 2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics . 474 (2): 653– 664. arXiv :0708.1752 . Bibcode :2007A& A...474..653V . doi :10.1051/0004-6361:20078357 .
1 2 3 4 5 6 7 Butler, R. Paul; et al. (2004). "A Neptune-Mass Planet Orbiting the Nearby M Dwarf GJ 436" . The Astrophysical Journal . 617 (1): 580– 588. arXiv :astro-ph/0408587 . Bibcode :2004ApJ...617..580B . doi :10.1086/425173 . Diakses tanggal 2009-12-26 .
1 2 Reid, I. Neill; et al. (July 2004), "Meeting the Cool Neighbors. VIII. A Preliminary 20 Parsec Census from the NLTT Catalogue", The Astronomical Journal , 128 (1): 463– 483, arXiv :astro-ph/0404061 , Bibcode :2004AJ....128..463R , doi :10.1086/421374
1 2 3 Cutri, R. M.; et al. (June 2003), 2MASS All Sky Catalog of point sources , NASA/IPAC, Bibcode :2003tmc..book.....C
1 2 "Query Result:LHS 310 -- High proper-motion Star" . SIMBAD Astronomical Object Database . Centre de Données astronomiques de Strasbourg . Diarsipkan dari asli tanggal 2016-03-04. Diakses tanggal 2007-11-28 .
↑ Wilson, Ralph Elmer (1953), General Catalogue of Stellar Radial Velocities , Washington: Carnegie Institution of Washington, Bibcode :1953QB901.W495.....
1 2 3 Johnson, H. M.; Wright, C. D. (1983). "Predicted infrared brightness of stars within 25 parsecs of the sun". Astrophysical Journal Supplement Series . 53 : 643– 711. Bibcode :1983ApJS...53..643J . doi :10.1086/190905 . —see page 673.
↑ Maness, H. L.; et al. (January 2007), "The M Dwarf GJ 436 and its Neptune-Mass Planet", The Publications of the Astronomical Society of the Pacific , 119 (851): 90– 101, arXiv :astro-ph/0608260 , Bibcode :2007PASP..119...90M , doi :10.1086/510689
↑ Bean, Jacob L.; Benedict, G. Fritz; Endl, Michael (2006). "Metallicities of M Dwarf Planet Hosts from Spectral Synthesis". The Astrophysical Journal (abstract). 653 (1): L65 – L68 . arXiv :astro-ph/0611060 . Bibcode :2006ApJ...653L..65B . doi :10.1086/510527 . —for the metallicity , note that
10
−
0.32
=
0.48
{\displaystyle {\begin{smallmatrix}10^{-0.32}=0.48\end{smallmatrix}}}
or 48%
↑ Jenkins, J. S.; et al. (October 2009), "Rotational Velocities for M Dwarfs", The Astrophysical Journal , 704 (2): 975– 988, arXiv :0908.4092 , Bibcode :2009ApJ...704..975J , doi :10.1088/0004-637X/704/2/975
↑ Saffe, C.; Gómez, M.; Chavero, C. (2006). "On the Ages of Exoplanet Host Stars". Astronomy & Astrophysics . 443 (2): 609– 626. arXiv :astro-ph/0510092 . Bibcode :2005A& A...443..609S . doi :10.1051/0004-6361:20053452 .
↑ New Planet Found: Molten "Mars" Is "Right Around the Corner" Diarsipkan 2015-06-11 di Wayback Machine . , Dave Mosher, National Geographic News , 19 Juli 2012
Stevenson, Kevin B.; et al. (July 2012). "Two nearby sub-Earth-sized exoplanet candidates in the GJ 436 system". The Astrophysical Journal . arXiv :1207.4245 . Bibcode :2012ApJ...755....9S . doi :10.1088/0004-637X/755/1/9 .
Sherrod, P. Clay; Koed, Thomas L. (2003), A Complete Manual of Amateur Astronomy: Tools and Techniques for Astronomical Observations , Astronomy Series, Courier Dover Publications, hlm. 9, ISBN 0486428206 , diarsipkan dari asli tanggal 2023-08-06, diakses tanggal 2015-06-13
"The Colour of Stars" , Australia Telescope, Outreach and Education , Commonwealth Scientific and Industrial Research Organisation, December 21, 2004, diarsipkan dari asli tanggal 2012-03-10, diakses tanggal 2012-01-16