Warming early Mars with carbon dioxide clouds that scatter infrared radiation.

Science (New York, N.Y.) 278:5341 (1997) 1273-1276

Authors:

F Forget, RT Pierrehumbert

Abstract:

Geomorphic evidence that Mars was warm enough to support flowing water about 3.8 billion years ago presents a continuing enigma that cannot be explained by conventional greenhouse warming mechanisms. Model calculations show that the surface of early Mars could have been warmed through a scattering variant of the greenhouse effect, resulting from the ability of the carbon dioxide ice clouds to reflect the outgoing thermal radiation back to the surface. This process could also explain how Earth avoided an early irreversible glaciation and could extend the size of the habitable zone on extrasolar planets around stars.

On the global warping of a thin self-gravitating near Keplerian gaseous disk with application to the disk in NGC 4258

(1997)

Authors:

John CB Papaloizou, Caroline Terquem, Doug NC Lin

Seyfert Activity and Nuclear Star Formation in the Circinus Galaxy

ArXiv astro-ph/9709091 (1997)

Authors:

R Maiolino, A Krabbe, N Thatte, R Genzel

Abstract:

We present high angular resolution (0".15-0".5) near infrared images and spectroscopy of the Circinus galaxy, the closest Seyfert 2 galaxy known. The data reveal a non-stellar nuclear source at 2.2 microns. The coronal line region and the hot molecular gas emission extend for 20-50 pc in the ionization cone. The data do not show evidence for a point-like concentration of dark mass; we set an upper limit of 4*10^6 Mo to the mass of a putative black hole. We find evidence for a young nuclear stellar population, with typical ages between 4*10^7 and 1.5*10^8 yrs. The luminosity of the starburst inside a few hundred pc is comparable to the intrinsic luminosity of the Seyfert nucleus, and the two of them together account for most of the observed bolometric luminosity of the galaxy. Within the central 12 pc the starburst has an age of about 7*10^7 yrs and radiates about 2% of the luminosity of the active nucleus. We discuss the implications of these results for models that have been proposed for the starburst-AGN connection.

Bending Instabilities in Magnetized Accretion Discs

(1997)

Authors:

Vasso Agapitou, John CB Papaloizou, Caroline Terquem

Lower-Tropospheric Heat Transport in the Pacific Storm Track

Journal of the Atmospheric Sciences American Meteorological Society 54:11 (1997) 1533-1543

Authors:

Kyle L Swanson, Raymond T Pierrehumbert