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sprovođenje zakonom predviđenih postupaka u cilju otkrivanja carinskih prekršaja, privrednih prestupa i krivičnih dela i podnošenje prijava tužilaštvu ili drugim nadležnim državnim organima;

Carina also contains the naked-eye globular cluster NGC 2808. [11] Epsilon Carinae and Upsilon Carinae are double stars visible in small telescopes. 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;

Uprava za javni dug

Sana, H.; etal. (June 2010). "A MAD view of Trumpler 14". Astronomy & Astrophysics. 515. A26. arXiv: 1003.2208. Bibcode: 2010A&A...515A..26S. doi: 10.1051/0004-6361/200913688. S2CID 119294869. Webb reveals emerging stellar nurseries and individual stars that are completely hidden in visible-light pictures. Because of Webb’s sensitivity to infrared light, it can peer through cosmic dust to see these objects. Protostellar jets, which emerge clearly in this image, shoot out from some of these young stars. The youngest sources appear as red dots in the dark, dusty region of the cloud. Objects in the earliest, rapid phases of star formation are difficult to capture, but Webb’s extreme sensitivity, spatial resolution, and imaging capability can chronicle these elusive events. 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. Typhoon Nida (2016), a 2016 Pacific typhoon known as Severe Tropical Storm Carina in the Philippines a b c Car Repair Manual–Carina/Celica. Maidenhead, Berkshire, UK.: Autodata. pp.6–7, History and Identification. (1981).

From China (especially northern China), the stars of Carina can barely be seen. The star Canopus (the south polar star in Chinese astronomy) was located by Chinese astronomers in the Vermilion Bird of the South (南方朱雀, Nán Fāng Zhū Què). The rest of the stars were first classified by Xu Guanggi during the Ming dynasty, based on the knowledge acquired from western star charts, and placed among The Southern Asterisms (近南極星區, Jìnnánjíxīngōu). [ clarification needed]

Poreska uprava

Frommert, Hartmut & Kronberg, Christine (6 May 2001). "Collinder 228". SEDS.org . Retrieved 29 November 2016. of people spoke only English at home. Other languages spoken at home included Mandarin 1.8%, Cantonese 1.3%, Greek 1.3% and Russian 0.9%.

There are several other stars above magnitude 3 in Carina. Beta Carinae, traditionally called Miaplacidus, is a blue-white-hued star of magnitude 1.7, 111 light-years from Earth. Epsilon Carinae is an orange-hued giant star similarly bright to Miaplacidus at magnitude 1.9; it is 630 light-years from Earth. Another fairly bright star is the blue-white-hued Theta Carinae; it is a magnitude 2.7 star 440 light-years from Earth. Theta Carinae is also the most prominent member of the cluster IC 2602. Iota Carinae is a white-hued supergiant star of magnitude 2.2, 690 light-years from Earth. [3] This object is currently the most massive star that can be studied in great detail, because of its location and size. Several other known stars may be more luminous and more massive, but data on them is far less robust. (Caveat: Since examples such as the Pistol Star have been demoted by improved data, one should be skeptical of most available lists of "most massive stars". In 2006, Eta Carinae still had the highest confirmed luminosity, based on data across a broad range of wavelengths.) Stars with more than 80 times the mass of the Sun produce more than a million times as much light as the Sun. They are quite rare—only a few dozen in a galaxy as big as ours—and they flirt with disaster near the Eddington limit, i.e., the outward pressure of their radiation is almost strong enough to counteract gravity. Stars that are more than 120 solar masses exceed the theoretical Eddington limit, and their gravity is barely strong enough to hold in its radiation and gas, resulting in a possible supernova or hypernova in the near future. In its third incarnation, the Carina followed the fashion of the time with a still more angular and four-square design (two-square headlights version also available). [16] The car followed its predecessors in retaining a front-engine rear-wheel-drive configuration even though by then competitor manufacturers were following a trend of switching to front-wheel drive in this class. In addition to the petrol-engined versions, the Carina was later (February 1982) offered with the option of an 1839cc 1C diesel engine, for which a power output of 65PS (48kW) at 4500rpm was claimed - in markets where fuel pricing and availability rendered this model appropriate.The more massive member of the pair is an O3.5 main sequence star. The spectrum shows some ionized nitrogen and helium emission lines, indicating some mixing of fusion products to the surface and a strong stellar wind. The mass calculated from apsidal motion of the orbits is 40 to 60 M ☉. This is somewhat lower than expected from evolutionary modelling of a star with its observed parameters. [45] Rear view of Toyota Carina 1500 SG (AA60) Alternative version of Toyota Carina A60 with single square headlights 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. Extremly low overhead. Carina sit besides the core data path and provide raw disk performance to applications. Eta Carinae's effects on the nebula can be seen directly. Dark globules and some other less visible objects have tails pointing directly away from the massive star. The entire nebula would have looked very different before the Great Eruption in the 1840s surrounded Eta Carinae with dust, drastically reducing the amount of ultraviolet light it put into the nebula.

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