how is it classified?
Eta Carinae A is classified as a luminous blue variable (LBV) due to the distinctive spectral and brightness variations.
Eta Carinae
Eta Carinae A is classified as a luminous blue variable (LBV) due to the distinctive spectral and brightness variations. 
where could be found hii emission nebula regions Sometimes several hundred light-years across, are often associated with giant molecular clouds what does this region mean? It is a region of interstellar atomic hydrogen that is ionized how did it get the name? The term H II is pronounced "H two" by astronomers. "H" is the chemical symbol for hydrogen, and "II" is the Roman numeral for 2. what are it's features? It vary greatly in their physical properties, their size is also known as the Stromgren radius and essentially depends on the intensity of the source of ionising photons and the density of the region, their densities range from over a million particles per cm³ in the ultra-compact H II regions to only a few particles per cm³ in the largest and most extended regions how is it distributed? The reason H II regions rarely appear in elliptical galaxies is that ellipticals are believed to form through galaxy mergers. In galaxy clusters, such mergers are frequent. does it face any problems? UNANSWERABLE which are the special regions it has? Orion Nebula, the Eta Carinae Nebula, and the Berkeley 59 / Cepheus OB4 Complex what is the second one about? It is also known as the Grand Nebula in Carina,  is a large complex area of bright and dark nebulosity in the constellation Carina who discovered it? Nicolas-Louis de Lacaille
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Eta Carinae [SEP] Classification
It does not currently lie on the S Doradus instability strip, although it is unclear what the temperature or spectral type of the underlying star actually is, and during its Great Eruption it was much cooler than a typical LBV outburst, with a middle-G spectral type. The 1890 eruption may have been fairly typical of LBV eruptions, with an early F spectral type, and it has been estimated that the star may currently have an opaque stellar wind, forming a pseudo-photosphere with a temperature of 9,000–10,000 K.