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First Paper from Gemini/HST Galaxy Survey: It Takes More Than Aging to Shape A Galaxy

Can galaxies observed at very high redshifts (at a time when the universe was a fraction of its current age) evolve to look like today's nearby galaxies simply by growing older? The answer is no according to an international team of scientists led by Inger Jørgenson (Gemini Observatory) who used GMOS on Gemini North, combined with HST imaging data to survey distant galaxies and chart their evolution.

100th Gemini Paper Reveals White Dwarf Progenitors are Prolific Mass Expellers

A long-standing problem in understanding the evolution of stars has been determining the nature of the stellar progenitors for white dwarf stars. In particular, astronomers want to know how a rather massive star (up to seven times the mass of the Sun) can lose enough mass to become a white dwarf. Key questions include: Which main-sequence stars eventually end their life as white dwarfs? How much mass do they lose in late evolutionary stages? What process allows this to occur?

Gemini Observatory Welcomes 2005 with Release of Galactic Fireworks Image

December 31, 2005

New Clouds Add to Titan's Mystery

En Español - Versión adaptada en Chile

Media Contacts:

Peter Michaud
Gemini Observatory

Phone: 808/974-2510
E-mail: pmichaud@gemini.edu

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