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- Q3270240 subject Q6504869.
- Q3270240 subject Q6859831.
- Q3270240 subject Q7009482.
- Q3270240 subject Q8293947.
- Q3270240 subject Q8480536.
- Q3270240 subject Q8790837.
- Q3270240 abstract "Iota Trianguli Australis (ι TrA, ι Trianguli Australis) is a triple star system in the constellation Triangulum Australe. It is approximately 132 light years from Earth.It shows itself to be composed of a yellow and a white star when seen though a 7.5 cm telescope.The primary component, Iota Trianguli Australis A, is a spectroscopic binary with a mean apparent magnitude of +5.28. Both components of the binary star are yellow-white F-type stars and they have an orbital period of 39.8 days. One of the components of the binary is also classified as a Gamma Doradus type variable star, and the binary's brightness varies by 0.12 magnitudes over a period of 1.45 days. The third component of the star system, Iota Trianguli Australis B, is a 10th magnitude star, 20 arcseconds away from the primary.".
- Q3270240 wikiPageWikiLink Q10422.
- Q3270240 wikiPageWikiLink Q111130.
- Q3270240 wikiPageWikiLink Q124313.
- Q3270240 wikiPageWikiLink Q1493194.
- Q3270240 wikiPageWikiLink Q179600.
- Q3270240 wikiPageWikiLink Q2.
- Q3270240 wikiPageWikiLink Q22066400.
- Q3270240 wikiPageWikiLink Q2703.
- Q3270240 wikiPageWikiLink Q50053.
- Q3270240 wikiPageWikiLink Q531.
- Q3270240 wikiPageWikiLink Q555846.
- Q3270240 wikiPageWikiLink Q595871.
- Q3270240 wikiPageWikiLink Q6243.
- Q3270240 wikiPageWikiLink Q6504869.
- Q3270240 wikiPageWikiLink Q6859831.
- Q3270240 wikiPageWikiLink Q7009482.
- Q3270240 wikiPageWikiLink Q8293947.
- Q3270240 wikiPageWikiLink Q8480536.
- Q3270240 wikiPageWikiLink Q850950.
- Q3270240 wikiPageWikiLink Q8790837.
- Q3270240 wikiPageWikiLink Q8928.
- Q3270240 comment "Iota Trianguli Australis (ι TrA, ι Trianguli Australis) is a triple star system in the constellation Triangulum Australe. It is approximately 132 light years from Earth.It shows itself to be composed of a yellow and a white star when seen though a 7.5 cm telescope.The primary component, Iota Trianguli Australis A, is a spectroscopic binary with a mean apparent magnitude of +5.28. Both components of the binary star are yellow-white F-type stars and they have an orbital period of 39.8 days.".
- Q3270240 label "Iota Trianguli Australis".