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2006, Siegfried Röser, Reviews in Modern Astronomy, The Many Facets of the Universe, page 187:First, the envelope, especially the material closest to the center, begins to warm up to an eventual temperature of ≈ 100 - 200 K. Now known as a “hot corino,” the warmed portion of the envelope becomes chemically quite different from the cooler outer part
2006, Publications of the Astronomical Society of Japan:Bottinelli et al. (2004a) named the hot region emitting the HCOOCH3 lines as a hot corino.
2013, Q. Ashton Acton, quoting National Center for Scientific Research, “Astrophysics research”, in Issues in Astronomy and Astrophysics, page 773:According to the news editors, the researchers concluded: “The similarity of the ratios derived in the hot corino and in the added absorbing layer suggests that water formed before the gravitational collapse of the protostar, contrary to formaldehyde and methanol, which formed later once the CO molecules had depleted on the grains.”