Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-09-12
Astrophys.J.599:992-996,2003
Astronomy and Astrophysics
Astrophysics
6 pages (emulateapj5) with 4 figures; accepted by The Astrophysical Journal
Scientific paper
10.1086/379537
We draw attention to the close relationship between the anisotropy parameter beta(r) for stellar orbits in elliptical galaxies and the temperature profile T(r) of the hot interstellar gas. For nearly spherical galaxies the gas density can be accurately determined from X-ray observations and the stellar luminosity density can be accurately found from the optical surface brightness. The Jeans equation and hydrostatic equilibrium establish a connection between beta(r) and T(r) that must be consistent with the observed stellar velocity dispersion. Purely optical observations of the bright elliptical galaxy NGC 4472 indicate beta(r) < 0.35 within the effective radius. However, the X-ray gas temperature profile T(r) for NGC 4472 requires significantly larger anisotropy, beta = 0.6 - 0.7, about twice the optical value. This strong preference for radial stellar orbits must be understood in terms of the formation history of massive elliptical galaxies. Conversely, if the smaller, optically determined anisotropy is indeed correct, we are led to the important conclusion that the temperature profile T(r) of the hot interstellar gas in NGC 4472 must differ from that indicated by X-ray observations, or that the hot gas is not in hydrostatic equilibrium.
Brighenti Fabrizio
Mathews William G.
No associations
LandOfFree
Stellar Orbits and the Interstellar Gas Temperature in Elliptical Galaxies does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Stellar Orbits and the Interstellar Gas Temperature in Elliptical Galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stellar Orbits and the Interstellar Gas Temperature in Elliptical Galaxies will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-166676