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==Distance== | ==Distance== | ||
In 1991, Gliese ''et al'' gave ] (πp) as 121.8 ± 3.0 ].<ref name="Gliese1991">{{cite book|last1=Gliese|first1=W.|last2=Jahreiß|first2=H.|title=Preliminary Version of the Third Catalogue of Nearby Stars|date=1991|chapter=GI 338|url=http://webviz.u-strasbg.fr/viz-bin/VizieR-5?-source=V/70A&Name=Gl%20338}}</ref> In 1995, van Altena gave parallax as 122.1 ± 2.9 mas.<ref name="van Altena1995"></ref> In 2014, Dittman ''et al'' gave parallax as 130.60 ± 3.60 mas.{{r|Dittmann2014}} | In 1991, Gliese ''et al'' gave ] (πp) as 121.8 ± 3.0 ].<ref name="Gliese1991">{{cite book|last1=Gliese|first1=W.|last2=Jahreiß|first2=H.|title=Preliminary Version of the Third Catalogue of Nearby Stars|date=1991|chapter=GI 338|url=http://webviz.u-strasbg.fr/viz-bin/VizieR-5?-source=V/70A&Name=Gl%20338}}</ref> In 1995, van Altena gave parallax as 122.1 ± 2.9 mas.<ref name="van Altena1995"></ref> In 2014, Dittman ''et al'' gave parallax as 130.60 ± 3.60 mas.{{r|Dittmann2014}} | ||
==See also== | |||
*] | |||
==References== | ==References== |
Revision as of 09:03, 23 June 2018
GJ 1151 is a red dwarf star of spectral type M4.5V, located in constellation Ursa Major at 26.7 light-years from Earth.
Distance
In 1991, Gliese et al gave parallax (πp) as 121.8 ± 3.0 mas. In 1995, van Altena gave parallax as 122.1 ± 2.9 mas. In 2014, Dittman et al gave parallax as 130.60 ± 3.60 mas.
See also
References
- ^ VizieR, Yale Trigonometric Parallaxes, Fourth Edition (van Altena+ 1995)
- Gliese, W.; Jahreiß, H. (1991). "GI 338". Preliminary Version of the Third Catalogue of Nearby Stars.
- Dittmann, Jason A.; Irwin, Jonathan M.; Charbonneau, David; Berta-Thompson, Zachory K. (2014). "TRIGONOMETRIC PARALLAXES FOR 1507 NEARBY MID-TO-LATE M DWARFS". The Astrophysical Journal. 784 (2): 156. arXiv:1312.3241. Bibcode:2014ApJ...784..156D. doi:10.1088/0004-637X/784/2/156. ISSN 0004-637X.
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Italic are systems without known trigonometric parallax. |
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