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Cooper, Ian; etal. (2008). The Night Sky Observer's Guide. Volume 3: The Southern Skies. Willmann-Bell. p.52. ISBN 978-0-943396-89-7. Toyota Carina 1600GT 4-door sedan (TA12), showing distinctive taillights 1975 Toyota Carina 1600GT hardtop coupe (TA17) with horizontal taillights Caringbah is a suburb in Southern Sydney, in the state of New South Wales, Australia. Caringbah is 24 kilometres (15mi) south of the Sydney central business district in the local government area of Sutherland Shire. a b c Car Repair Manual–Carina/Celica. Maidenhead, Berkshire, UK.: Autodata. pp.6–7, History and Identification. (1981). 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]

Find sources: "Carina"constellation– news · newspapers · books · scholar · JSTOR ( July 2021) ( Learn how and when to remove this template message) Sana, H.; etal. (November 2014). "Southern Massive Stars at High Angular Resolution: Observational Campaign and Companion Detection". The Astrophysical Journal Supplement. 215 (1). 15. arXiv: 1409.6304. Bibcode: 2014ApJS..215...15S. doi: 10.1088/0067-0049/215/1/15. S2CID 53500788.In October 1982, the Turbo DOHC engine (3T-GTEU, 1770cc and 160PS (118kW) in the Touring Super Coupé trim level) with the "GT-TR" trim level was added. Celica and Corona were released with the same powerplant simultaneously. Conversely, the 18R-GEU-engined 2000GT hardtop coupe was no longer available, and was replaced by the next-generation Carina ED four-door hardtop in 1985. hemijsko-tehnološka i druga ispitivanja uzoraka robe u carinskoj laboratoriji, u svrhu pravilnog svrstavanja robe po Carinskoj tarifi; in NGC 3603; Algol variable, Δ V = 0.45 m, P = 3.77d both components among the most luminous and massive stars known Caringbah South is a small district made up mostly of small businesses specialising in professional services.

Gräfener, G. & Hamann, W.-R. (May 2008). "Mass loss from late-type WN stars and its Z-dependence. Very massive stars approaching the Eddington limit". Astronomy & Astrophysics. 482 (3): 945–960. arXiv: 0803.0866. Bibcode: 2008A&A...482..945G. doi: 10.1051/0004-6361:20066176. S2CID 16025012.a b c d e f "NGC 3372". The NGC/IC Project. Archived from the original on 28 May 2009 . Retrieved 29 November 2016. SIMBAD Astronomical Database". Centre de Données astronomiques de Strasbourg . Retrieved 2007-01-02. Called the Cosmic Cliffs, Webb’s seemingly three-dimensional picture looks like craggy mountains on a moonlit evening. In reality, it is the edge of the giant, gaseous cavity within NGC 3324, and the tallest “peaks” in this image are about 7 light-years high. The cavernous area has been carved from the nebula by the intense ultraviolet radiation and stellar winds from extremely massive, hot, young stars located in the center of the bubble, above the area shown in this image. In August 1979, the front of the vehicle received a major change that now included four headlamp lights rather than the previous setup, with the Van remaining with four round lamps. The rear received a changed license plate mounting to give it a new style. 3T-EU and 21R-U engines were now available with the four-speed automatic transmission. These two, along with the 18R-GEU, were now the only engines offered (in Japan). The rear suspension became of the semi-trailing type, becoming the A50 series Carina in the process. The Super Deluxe two-door sedan was discontinued, as was the 1400 Van. The 1600 Van received the 12T-J engine and the option of an automatic transmission, along with a chassis code now in line with the remainder of the Carina range (TA49V). If nodes fails, carina will automatically detach the local volume from pods thus pods can be rescheduled.

In 1971, the Carina 1600GT was introduced as an alternative to the Corona-based Toyota 1600GT, using a 2T-G type 1600 DOHC engine shared with the Celica GT. The Corona GT was exclusive to Toyopet Store locations, while the Carina 1600GT was exclusive to Toyota Store locations, and the Celica GT was exclusive to Toyota Corolla Store locations. The chassis code was A10, with A15, 17 and 18 being reserved for hardtop coupés. Excepting the anomalous RA16 hardtop, A16 and 19 were used on vans (utility wagons). Beginning in 1975, A30-series numbers were used for some hardtop coupés. The wagons/vans of the first generation were not regularly exported. Carina vans entered production in December 1975. [4] Carina is in the southern sky quite near the south celestial pole, making it never set (circumpolar) for most of the southern hemisphere. Due to precession of Earth's axis, by the year 4700 the south celestial pole will be in Carina. Three bright stars in Carina will come within 1 degree of the southern celestial pole and take turns as the southern pole star: Omega Carinae (mag 3.29) in 5600, Upsilon Carinae (mag 2.97) in 6700, and Iota Carinae (mag 2.21) in 7900. About 13,860 CE, the bright Canopus (−0.7) will have a greater declination than −82°. [17] Namesakes [ edit ]In May 1984, the Carina FF four-door sedan (T150 series) was introduced. The styling echoed that of the previous generation, using four headlights and grille setup. The upper trim level model has aerodynamic headlight option. Rather than replace the entire line-up all at once because sales of the previous generation were still good, Toyota gradually introduced the replacement Coupé, Van (wagon) models in stages. The 1,800cc engine is electronically controlled distributorless ignition, and a 2,000cc diesel is added. Other 1600 cc EFI "4A-ELU" engine, and a carburetor is used on the 1500 cc with "3A-LU" type engine. The 1800SE models were still offered. Wolf–Rayet star and rotating ellipsoidal variable, Δ V = 0.04 m, P = 4.76d; one of the most luminous stars known in Collinder 228; Wolf–Rayet star, V max = 6.46 m, V min = 6.49 m, P = 4.76d; one of the most luminous stars known WR 25 is a binary system in the central portion of the Carina Nebula, a member of the Trumpler 16 cluster. The primary is a Wolf–Rayet star, possibly the most luminous star in the galaxy. The secondary is hard to detect but thought to be a luminous OB star.