Výsledky vyhledávání - "Unterguggenberger, S."

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Comparison of VLT/X-shooter OH and O2 rotational temperatures with consideration of TIMED/SABER emission and temperature profiles

Autor: Noll, S., Kausch, W., Kimeswenger, S., Unterguggenberger, S., Jones, A. M.

Rotational temperatures Trot derived from lines of the same OH band are an important method to study the mesopause region near 87 km. To measure realistic temperatures, the rotational level populations have to be in local thermodynamic equilibrium (L

Externí odkaz: http://arxiv.org/abs/1604.03961

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The effects of ram-pressure stripping on the internal kinematics of simulated spiral galaxies

Autor: Kronberger, T., Kapferer, W., Unterguggenberger, S., Schindler, S., Ziegler, B. L.

We investigate the influence of ram-pressure stripping on the internal gas kinematics of simulated spiral galaxies. Additional emphasis is put on the question of how the resulting distortions of the gaseous disc are visible in the rotation curve and/

Externí odkaz: http://arxiv.org/abs/0803.3690

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On the influence of ram-pressure stripping on the star formation of simulated spiral galaxies

Autor: Kronberger, T., Kapferer, W., Ferrari, C., Unterguggenberger, S., Schindler, S.

We investigate the influence of ram-pressure stripping on the star formation and the mass distribution in simulated spiral galaxies. Special emphasis is put on the question where the newly formed stars are located. The stripping radius from the simul

Externí odkaz: http://arxiv.org/abs/0801.3759

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The unusual Nova Cygni 2006 (V2362 Cyg)

Autor: Kimeswenger, S., Dalnodar, S., Knapp, A., Schafer, J., Unterguggenberger, S., Weiss, S.

Context: Optical nova lightcurves often have structures, such as rapid declines and recoveries, due to nebular or dusty phases of the ejecta. Nova Cygni 2006 (V2362 Cyg) underwent an unusual brightening after an early rapid decline. The shape of the

Externí odkaz: http://arxiv.org/abs/0801.2379

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