Theoretical astrophysics and plasma physics at RPC

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Supernovae and the intergalactic medium

GAS AND GALAXY EVOLUTION: A CONFERENCE IN HONOR OF THE 20TH ANNIVERSARY OF THE VLA 240 (2001) 355-362
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The black hole mass vs bulge mass relationship in spiral galaxies

GALAXIES AND THEIR CONSTITUENTS AT THE HIGHEST ANGULAR RESOLUTIONS (2001) 58-61

Authors:

A Marconi, D Axon, J Atkinson, J Binney, A Capetti, M Carollo, L Dressel, H Ford, J Gerssen, M Hughes, D Macchetto, W Maciejewski, M Merrifield, C Scarlata, W Sparks, M Stiavelli, Z Tsvetanov, R van der Marel
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Tidally–Induced Angular Momentum Transport in Disks

Symposium - International Astronomical Union Cambridge University Press (CUP) 200 (2001) 406-409
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Dynamical Relaxation and Massive Extrasolar Planets

(2000)

Authors:

JCB Papaloizou, Caroline Terquem
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The black hole mass vs bulge mass relationship in spiral galaxies

ArXiv astro-ph/0012155 (2000)

Authors:

A Marconi, D Axon, J Atkinson, J Binney, A Capetti, M Carollo, L Dressel, H Ford, J Gerssen, M Hughes, D Macchetto, W Maciejewski, M Merrifield, C Scarlata, W Sparks, M Stiavelli, Z Tsvetanov, R van der Marel

Abstract:

We describe an on-going HST program aimed at determining the relationship between the nuclear black hole mass and bulge mass in spiral galaxies. We have selected a volume limited sample of 54 nearby spiral galaxies for which we already have ground based emission line rotation curves, CCD surface photometry and radio maps. We are now obtaining HST/STIS longslit observations of each of the galaxies in the sample in order to determine the nuclear Halpha rotation curve at high (~0.1") spatial resolution. We will use these data to measure the unresolved dark mass concentration at the nucleus of each object. Here we show the first results from observations of objects in the sample.
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