OGLE-2006-BLG-109L in 2008 by a research team using Microlensing. Optical Gravitational Lensing Experiment or OGLE 47 Ursae Majoris b OGLE-2005-BLG-390Lb...
3 KB (191 words) - 07:39, 26 February 2023
OGLE-2006-BLG-109L (where the last 'L' stands for lens) is a dim magnitude 17 M0V galactic bulge star approximately 4,920 light-years away in the constellation...
6 KB (342 words) - 15:22, 7 March 2024
Gravitational Lensing Experiment or OGLE 47 Ursae Majoris b OGLE-2005-BLG-390Lb OGLE-2006-BLG-109Lb "OGLE-2006-BLG-109L c". NASA Exoplanet Exploration. Retrieved...
4 KB (226 words) - 12:07, 5 January 2024
Optical Gravitational Lensing Experiment (redirect from OGLE)
detected by the gravitational microlensing method, year stands for OGLE season, BLG means that an event detected is in the Galactic BuLGe, and the following...
16 KB (1,115 words) - 18:18, 3 September 2024
examples include OGLE-2005-BLG-071Lb, OGLE-2005-BLG-390Lb, OGLE-2005-BLG-169Lb, two exoplanets around OGLE-2006-BLG-109L, and MOA-2007-BLG-192Lb. Notably...
54 KB (7,159 words) - 07:19, 26 August 2024
Chi Scorpii (redirect from 17 Sco b)
Bibcode:2020A&A...644A...1T. doi:10.1051/0004-6361/202038285. 17 Sco b on exoplanet.eu Kaler, James B. (August 12, 2016), "Chi and Psi Scorpii", Stars, University...
8 KB (597 words) - 05:55, 21 August 2024
S2CID 18759600. Kozok, J. R. (September 1985), "Photometric observations of emission B-stars in the southern Milky Way", Astronomy and Astrophysics Supplement Series...
9 KB (784 words) - 04:26, 21 August 2024
Mu2 Scorpii (redirect from Mu2 Scorpii b)
Centaurus–Lupus subgroup of the Scorpius–Centaurus association. This is a blue-white, B-type subgiant star with a stellar classification of B2 IV. It has an estimated...
13 KB (931 words) - 04:11, 15 November 2024
Omega1 Scorpii (category B-type main-sequence stars)
Strasbourg. Retrieved 2016-09-25. Jilinski, E.; et al. (March 2006), "Radial velocity measurements of B stars in the Scorpius-Centaurus association", Astronomy...
10 KB (765 words) - 14:20, 8 October 2023
Rho Scorpii (category B-type subgiants)
Scorpius OB association. It has two components, designated Rho Scorpii A and B. Rho Scorpii A is itself a single-lined spectroscopic binary whose components...
13 KB (983 words) - 07:44, 2 July 2024
K2-24 K2-33 LSS 4067 MOA-2008-BLG-310L MXB 1735-44 OAO 1657-415 OGLE-2005-BLG-071L OGLE-2005-BLG-390L OGLE-2006-BLG-109L Oph 162225-240515 Pismis 24-1...
7 KB (658 words) - 15:51, 8 November 2024
données astronomiques de Strasbourg. Retrieved 2016-09-22. Whittet, D. C. B. (February 1988), "On the nature and environment of Omicron Scorpii", Monthly...
8 KB (615 words) - 06:00, 21 August 2024
Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976. Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog", The Astronomical...
8 KB (561 words) - 05:23, 21 August 2024
Union, p. 57, Bibcode:1967IAUS...30...57E. da Silva, L.; et al. (November 2006), "Basic physical parameters of a selected sample of evolved stars", Astronomy...
6 KB (427 words) - 23:28, 1 May 2024
869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976. Kaler, James B. (August 12, 2016), "Chi and Psi Scorpii", Stars, University of Illinois,...
8 KB (644 words) - 04:31, 21 August 2024
star is similar to the light curve of a candidate exoplanet, KIC 10403228 b, which may have been caused by a "tilted ring system" orbiting the planet...
7 KB (438 words) - 01:19, 30 October 2024
K2-24 K2-33 LSS 4067 MOA-2008-BLG-310L MXB 1735-44 OAO 1657-415 OGLE-2005-BLG-071L OGLE-2005-BLG-390L OGLE-2006-BLG-109L Oph 162225-240515 Pismis 24-1...
6 KB (548 words) - 01:29, 29 October 2024