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Infrared profile of central region of our Galaxy at 2.47 µm (1977)

ITO, K. ; MATSUMOTO, T. ; UYAMA, K.

[s.l.] : Nature Publishing Group

Nature 265 (1977), S. 517-518

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ISSN: 1476-4687

Source: Nature Archives 1869 - 2009

Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics

Notes: [Auszug] Fig. 1 Isophoto of the observed surface brightness of our Galaxy. The shaded area (bottom right) indicates the field of view used (HMBW). Fig. 2 Longitude dependence of 2.4-µm surface brightness on the galactic plane. Newly obtained data are shown by filled circles while open circles and ...

Type of Medium: Electronic Resource

URL: http://dx.doi.org/10.1038/265517a0

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