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Gould, B. A. "Uranometria Argentina". Reprinted and updated by Pilcher, F. Archived from the original on 2012-02-27 . Retrieved 2010-07-19. ispitivanje u ime drugih carinskih administracija (zamolnim putem), u skladu sa međunarodnim ugovorima; Polynesian peoples had no name for the constellation in particular, though they had many names for Canopus. Maíz Apellániz, J.; etal. (May 2016). "The Galactic O-Star Spectroscopic Survey (GOSSS). III. 142 Additional O-type Systems". The Astrophysical Journal Supplement Series. 224 (1). 4. arXiv: 1602.01336. Bibcode: 2016ApJS..224....4M. doi: 10.3847/0067-0049/224/1/4. S2CID 55658165. Within the large bright nebula is a much smaller feature, immediately surrounding Eta Carinae itself, known as the Homunculus Nebula (from Latin meaning Little Man). It is believed to have been ejected in an enormous outburst in 1841 which briefly made Eta Carinae the second-brightest star in the sky.

The nebula has within its boundaries the large Carina OB1 association and several related open clusters, including numerous O-type stars and several Wolf–Rayet stars. Carina OB1 encompasses the star clusters Trumpler 14 and Trumpler 16. Trumpler 14 is one of the youngest known star clusters at half a million years old. Trumpler 16 is the home of WR 25, currently the most luminous star known in our Milky Way galaxy [ citation needed], together with the less luminous but more massive and famous Eta Carinae star system and the O2 supergiant HD 93129A. Trumpler 15, Collinder 228, Collinder 232, NGC 3324, and NGC 3293 are also considered members of the association. NGC 3293 is the oldest and furthest from Trumpler 14, indicating sequential and ongoing star formation. Carina is known for its namesake nebula, NGC 3372, [8] discovered by French astronomer Nicolas-Louis de Lacaille in 1751, which contains several nebulae. The Carina Nebula overall is an extended emission nebula approximately 8,000 light-years away and 300 light-years wide that includes vast star-forming regions. [9] It has an overall magnitude of 8.0 [6] and an apparent diameter of over 2 degrees. [3] Its central region is called the Keyhole, or the Keyhole Nebula. This was described in 1847 by John Herschel, and likened to a keyhole by Emma Converse in 1873. [10] The Keyhole is about seven light-years wide and is composed mostly of ionized hydrogen, with two major star-forming regions. The Homunculus Nebula is a planetary nebula visible to the naked eye that is being ejected by the erratic luminous blue variable star Eta Carinae, the most massive visible star known. Eta Carinae is so massive that it has reached the theoretical upper limit for the mass of a star and is therefore unstable. It is known for its outbursts; in 1840 it briefly became one of the brightest stars in the sky due to a particularly massive outburst, which largely created the Homunculus Nebula. Because of this instability and history of outbursts, Eta Carinae is considered a prime supernova candidate for the next several hundred thousand years because it has reached the end of its estimated million-year life span. [9] Thomas Holt (1811–88) owned most of the land that stretched from Sutherland to Cronulla in the 1860s. Most of the area around Miranda and Caringbah was used for market gardening from the 1880s. Caringbah was still used for orchards and farming until after World War II. The railway line to Cronulla opened in 1939. [4] Commercial area [ edit ]This generation was released in May 1988. The exterior sheet metal received rounded contours, as was in line with the fashionable design of products at that time. The Surf (wagon) and Van versions also underwent a full model change to bring them in line with their siblings. 4S-Fi is an 1800cc engine type, 1600cc of the 4A-GE and the specification for higher-power higher-cam-4A-FHE car, 1500cc of the 5A-F type, 2000cc diesel-2C. The 3E engine was fitted to the 1500cc Van, which was also available with the 2000cc diesel 2C engine. [18]

MIRI was contributed by ESA and NASA, with the instrument designed and built by a consortium of nationally funded European Institutes (The MIRI European Consortium) in partnership with JPL and the University of Arizona. a b c Car Repair Manual–Carina/Celica. Maidenhead, Berkshire, UK.: Autodata. pp.6–7, History and Identification. (1981). possibly in Trumpler 15; irregular variable, V max = 8.2 m, V min = 9.9 m, one of the largest stars known izdavanje obaveštenja o primeni carinskih i drugih propisa iz nadležnosti Uprave carina i obavezujućih obaveštenja o svrstavanju i poreklu robe; In August 1989, the "G Limited" with the high-performance and high-compression 4A-GE engine is added; it has 140PS (103kW).

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inicijative za pokretanje postupka za vođenje pregovora i zaključivanje međunarodnih ugovora iz delokruga carinske službe i saradnja i razmena podataka sa stranim carinskim i drugim službama i međunarodnim organizacijama; Houk, Nancy & Cowley, Anne P. (1975). University of Michigan Catalogue of Two-Dimensional Spectral Types for the HD Stars. Volume 1. Declinations −90° to −53°. Department of Astronomy, University of Michigan. Bibcode: 1975mcts.book.....H. ISBN 978-0-8357-0331-4. Eta Carinae is the most prominent variable star in Carina, with a mass of approximately 100 solar masses and 4 million times as bright as the Sun. [3] It was first discovered to be unusual in 1677, when its magnitude suddenly rose to 4, attracting the attention of Edmond Halley. [6] Eta Carinae is inside NGC 3372, commonly called the Carina Nebula. [3] It had a long outburst in 1827, when it brightened to magnitude 1, only fading to magnitude 1.5 in 1828. Its most prominent outburst made Eta Carinae the equal of Sirius; it brightened to magnitude −1.5 in 1843. In the decades following 1843 it appeared relatively placid, having a magnitude between 6.5 and 7.9. [6] However, in 1998, it brightened again, though only to magnitude 5.0, a far less drastic outburst. Eta Carinae is a binary star, with a companion that has a period of 5.5 years; the two stars are surrounded by the Homunculus Nebula, which is composed of gas that was ejected in 1843. [3] sprovođenje mera carinskog nadzora i carinske kontrole koja obuhvata prethodne, preventivne i naknadne carinske kontrole nad carinskom robom, određene zakonom i drugim propisima; Kunitzsch, P., & Smart, T. (2006). A Dictionary of Modern star Names: A Short Guide to 254 Star Names and Their Derivations (2nd rev.ed.). Cambridge, MA: Sky Pub. p.25. ISBN 978-1-931559-44-7. {{ cite book}}: CS1 maint: multiple names: authors list ( link)

Samus, N. N.; Durlevich, O. V.; etal. (2012). "General Catalog of Variable Stars (GCVS database, version 2012Feb)" . Retrieved 2012-04-08. Starting with this generation, fuel injection was available optionally on top level models. In November 1977, the 3T-U 1,800cc engine emissions are updated. In May 1978, the GT 1600cc was added, and a three-speed automatic transmission became available. The 1600GT 2T-GEU engine was made to comply with the Showa 53 (1978) emissions regulation, while output improved from 110PS (81kW; 108hp) to 115PS (85kW; 113hp). The options list was updated to include a urethane bumper for impact improvement. Walborn, N. R. & Ingerson, T. E. (July 1977). "Structure in the Carina Nebula and Eta Carinae". Sky and Telescope. 54: 22–24. Bibcode: 1977S&T....54...22W. Widening and distortion of the carina is a serious radiological sign that usually indicates carcinoma of the lymph nodes around the region where the trachea divides. [ citation needed] Additional images [ edit ] Samus, N. N.; Durlevich, O. V.; etal. (2004). "Combined General Catalogue of Variable Stars (GCVS4.2)" . Retrieved 2012-04-08.

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Garner, Rob (8 July 2022). "NASA Shares List of Cosmic Targets for Webb Telescope's 1st Images". NASA . Retrieved 8 July 2022.

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