Anagram & Information om | Engelska ordet LBV
LBV
Antal bokstäver
3
Är palindrom
Nej
Sök efter LBV på:
Wikipedia
(Svenska) Wiktionary
(Svenska) Wikipedia
(Engelska) Wiktionary
(Engelska) Google Answers
(Engelska) Britannica
(Engelska)
(Svenska) Wiktionary
(Svenska) Wikipedia
(Engelska) Wiktionary
(Engelska) Google Answers
(Engelska) Britannica
(Engelska)
Exempel på hur man kan använda LBV i en mening
- The nature of the variation is somewhat unusual for an LBV; S Doradus is typically in an outburst state, with only occasional fades to the quiescent state that is typical of most stars in the class.
- Load Bearing Vest (LBV) – The vest could be the current standard-issue, second-generation, MOLLE fighting load carrier vest (FLC) or the late 1980s to early 1990s IIFS non-modular load bearing vest (LBV-88).
- Located about 5,300 light-years (1,560 parsecs) from Earth, it is a hypergiant luminous blue variable (LBV) star of spectral type B1-2 Ia-0ep that is one of the most luminous stars in the Milky Way.
- Apart from being co-credited on Haynes' 2004 solo record (released primarily through Surfdog Records and not officially counted in the current LBV catalogue system), Latino Buggerveil appears mainly to be a conduit for archival Butthole Surfers releases, as evinced by the reissue of the group's first two Alternative Tentacles releases on one CD and the rarities collection Humpty Dumpty LSD.
- Many luminous blue variables (LBVs) show Alpha Cygni-type variability during their quiescent (hot) phases, but the LBV classification is generally used in these cases.
- It contains the soft gamma repeater SGR 1806−20 and the luminous blue variable hypergiant LBV 1806−20, a candidate for the most luminous star in the Milky Way.
- Stars with sufficiently strong mixing from the core to the surface, due to the very large convective core, high metallicity, or additional rotational mixing, may skip the LBV phase and evolve directly from the hydrogen-rich WNh phase to the hydrogen-poor WN phase.
- 1 is the most notable as it contains the star cluster 1806-20 that includes the famous luminous blue variable star LBV 1806-20, the magnetar SGR 1806-20, two blue hypergiant stars, a supergiant O star, three Wolf-Rayet stars, two of them carbon-rich, and other young, massive stars.
Förberedelsen av sidan tog: 148,68 ms.