Titlebook: Spiral Galaxies in the Near-IR; Proceedings of the E Dante Minniti,Hans-Walter Rix Conference proceedings 1996 Springer-Verlag Berlin Heide

激勵

Photometric and Spectrophotometric Models in the NIRsed. One is a refined spectral synthesis of starbursts in the . band. Another model aims to predict synthetic spectra (continua and lines) and colors of starbursts and the Hubble Sequence from 220? to 5μm.

國家明智

踉蹌

裝飾

Colour Gradients in the Optical and Near-IRroadband colours are easy to obtain for large samples of objects, making them ideal for statistical studies. In this paper I use the radial distribution of the colours in galaxies, which gives more insight into the local processes driving the global colour differences than integrated colours. Almost

衰弱的心

脫水

Alopecia-Areata

jagged

defile

Imaging of Local Group Bulge Populations in the Near Infrarede from a globular cluster-aged stellar population. Giants with .. < -5 are found in M31, M32, and M33, and the HST imaging strongly supports the idea that ground-based observers are not being confused by blended images of stars. On the other hand, a direct measurement of the age of the Galactic bulg

惰性女人

Origin of Bulgesart of the spheroid formation process, that includes halo and bulge. In a more recently proposed scenario bulges form late, as a result of the dynamical evolution of a disk that is prone to develop a bar instability. Recent . and . results are reported that may help chosing among these two alternati