The Formation and Early Evolution of the Milky Way Galaxy

Author:

Buser Roland1

Affiliation:

1. Astronomisches Institut der Universität Basel, Venusstrasse 7, CH-4102 Binningen, Switzerland.

Abstract

Recent observations indicate that the Milky Way may have formed by aggregation of gas and stars from a reservoir of preexisting small galaxies in the local universe. The process probably began more than 12 billion years ago with material of different original angular momentum following two separate evolutionary lines, one into the slowly rotating halo and central bulge and the other into the rapidly rotating disk. The existence of distinct thick and thin disks shows that continuing mergers of satellite galaxies likely also determined the early evolution of the main structural component of the luminous Galaxy.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference104 articles.

1. A recent review of the Local Group is given by S. van den Bergh [ Astron. Astrophys. Rev. 9 273 (1999)].

2. The common length unit used in astronomy is the parsec (pc) derived from the (unit) parallactic second of arc angle subtended by the semimajor axis a of Earth's orbit (around the sun) as seen from a distance of 1 pc. Because a = 1.496 × 10 13 cm it follows that 1 pc = 3.086 × 10 13 km = 3.2615 light years; 1 kpc = 10 3 pc.

3. A dwarf satellite galaxy in Sagittarius

4. Here we consider only those components of the Galaxy which consist of luminous stars formed from gas and dust of ordinary matter. The dark matter component is discussed in other papers in this issue (11);

5. The Baryon Halo of the Milky Way: A Fossil Record of Its Formation

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