Titlebook: Infrared Astronomy with Arrays; The Next Generation Ian S. McLean Book 1994 Springer Science+Business Media Dordrecht 1994 Excel.Observator

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Infrared Astronomy with Arrays978-94-011-1070-9Series ISSN 0067-0057 Series E-ISSN 2214-7985

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The Mass Function of Faint Field Galaxiese consistent with the no-evolution or pure luminosity evolution models. The excess faint blue galaxies seen in the B band number counts at intermediate magnitudes are a result of a low normalization, and do not dominate the population until . ≈ 25. Extreme merging or excess dwarf models are not needed.

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Application of Near-IR Spectroscopy to the Study of the Stellar Content in Starburst Galaxiesd metallicity and ellipticals). Using proper IR spectral indices, which have been found to be powerful indicators of temperature in cool stars, some preliminary consideration on the dominant stellar population in the nuclear region of these galaxies are drawn.

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Astrophysics and Space Science Libraryhttp://image.papertrans.cn/i/image/466267.jpg

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Book 1994 of the Hilo conference, excitement was running high and everyone present was in favor of another meeting. I recall suggesting to Al Fowler that the next meeting could be in Tucson. Despite Al‘s reply to the effect that Hawaii was a much nicer location, a meeting was held in Tucson three years later

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