Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ap%26ss.265..213n&link_type=abstract
Astrophysics and Space Science, v. 265, Issue 1/4, p. 213-220 (1999).
Astronomy and Astrophysics
Astrophysics
32
Scientific paper
The status of the Galactic thick disk is reviewed. Consideration of the recent literature suggests that its vertical scale height and normalisation with respect to the thin disk remain uncertain to within a factor two, with values reported in the ranges 750-1500 pc, and 0.02-0.13, respectively. The bulk of the thick disk has kinematics (σU, σV, σW) = (65, 54, 38 km s-1), and lags the thin disk by some 40 km s-1; differences of opinion exists as to whether kinematics change with distance from the Galactic plane. The bulk of the thick disk has [Fe/H] ˜ -0.6, with little or no evidence for a vertical gradient. The question of gradients is critical for an understanding of thick disk cosmogony and needs closer attention. The reality of the so-called metal-weak thick disk (material having disklike kinematics and [Fe/H] ≤ -1.0) is also considered. The case for such material seems to be steadily growing: in the range -1.6 ≤ [Fe/H] ≤ -1.0, recent estimates suggest ρMWTD/ρHalo ˜ 0.1-0.3. While many workers regard the thick disk as a discrete entity, the caveat is made that this is a sufficient condition, but not one necessarily required by the observations. Best practice requires that both the discrete model and the alternative extended configuration be compared with observational data to examine the relative likelihood of their relevance. Recent theoretical advances are also discussed, together with the need for in situ measurements of the thick disk away from the Galactic plane.
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