Mu Arae
Appearance
Mu Arae sive μ Ara (aliter HD 160691) est stella pumilio flava constellationis Arae, a nobis annis luce mensis fere 50 distans, quam planetae ad minimum quattuor circumaguntur.
Planetae
[recensere | fontem recensere]Bibliographia
[recensere | fontem recensere]- Krzysztof Gozdziewski, Andrzej J. Maciejewski, Cezary Migaszewski, "On the extrasolar multi-planet system around HD160691" in Astrophysical Journal vol. 657 (2007) pp. 546-558
- F. Pepe, A.C.M. Correia, M. Mayor, O. Tamuz, W. Benz, J.-L. Bertaux, F. Bouchy, J. Couetdic, J. Laskar, C. Lovis, D. Naef, D. Queloz, N.C. Santos, J.-P. Sivan, D. Sosnowska, S. Udry, "The HARPS search for southern extra-solar planets. IX. mu Ara, a system with four planets" in Astronomy and Astrophysics vol. 462 (2006) pp. 769–776
- M. Soriano, S. Vauclair, "New seismic analysis of the exoplanet-host star Mu Arae" (2009) in Astronomy and Astrophysics divulganda
Nexus externi
[recensere | fontem recensere]Vicimedia Communia plura habent quae ad Mu Arae spectant. |
Data astronomica: "* mu. Ara" apud SIMBAD. "01434" apud ARICNS. |
Haec stipula ad astronomiam spectat. Amplifica, si potes! |