Zobrazeno 1 - 10
of 48
pro vyhledávání: '"Moellenhoff, C."'
Publikováno v:
Astron.Astrophys. 459 (2006) 703-716
We present a physical model that explains the two disparate observational facts: 1) the exponential vertical disc structure in the optical and NIR of the non-obscured part of the stellar disc and 2) the enhanced FIR/submm luminosity by about a factor
Externí odkaz:
http://arxiv.org/abs/astro-ph/0608196
We present corrections for the change in the apparent scalelengths, central surface brightnesses and axis ratios due to the presence of dust in pure disk galaxies, as a function of inclination, central face-on opacity in the B-band (tau^f_B) and wave
Externí odkaz:
http://arxiv.org/abs/astro-ph/0606562
Autor:
Jaeger, K., Ziegler, B. L., Boehm, A., Heidt, J., Moellenhoff, C., Hopp, U., Mendez, R. H., Wagner, S.
Publikováno v:
Astron.Astrophys. 422 (2004) 907-913
We have conducted an observing campaign with FORS at the ESO-VLT to explore the kinematical properties of spiral galaxies in distant galaxy clusters. Our main goal is to analyse transformation- and interaction processes of disk galaxies within the sp
Externí odkaz:
http://arxiv.org/abs/astro-ph/0406024
We present our project on galaxy evolution in the environment of distant rich clusters aiming at disentangling the importance of specific interaction and galaxy transformation processes from the hierarchical evolution of field galaxies. Spatially res
Externí odkaz:
http://arxiv.org/abs/astro-ph/0405081
Publikováno v:
Astrophys.J.598:L87,2003
We introduce our project on galaxy evolution in the environment of rich clusters aiming at disentangling the importance of specific interaction and galaxy transformation processes from the hierarchical evolution of galaxies in the field. Emphasis is
Externí odkaz:
http://arxiv.org/abs/astro-ph/0309267
Autor:
Heidt, J., Appenzeller, I., Gabasch, A., Jaeger, K., Seitz, S., Bender, R., Boehm, A., Snigula, J., Fricke, K. J., Hopp, U., Kuemmel, M., Moellenhoff, C., Szeifert, T., Ziegler, B., Drory, N., Mehlert, D., Moorwood, A., Nicklas, H., Noll, S., Saglia, R. P., Seifert, W., Stahl, O., Sutorius, E., Wagner, S. J.
Publikováno v:
Astron.Astrophys.398:49-62,2003
The FORS Deep Field project is a multi-colour, multi-object spectroscopic investigation of an approx. 7 times 7 region near the south galactic pole based mostly on observations carried out with the FORS instruments attached to the VLT telescopes. It
Externí odkaz:
http://arxiv.org/abs/astro-ph/0211044
Autor:
Mehlert, D., Noll, S., Appenzeller, I., Saglia, R. P., Bender, R., Boehm, A., Drory, N., Fricke, K. J., Gabasch, A., Heidt, J., Hopp, U., Jaeger, K., Moellenhoff, C., Seitz, S., Stahl, O., Ziegler, B.
Publikováno v:
Astron.Astrophys. 393 (2002) 809-820
Using a sample of 57 VLT FORS spectra in the redshift range 1.37
Externí odkaz:
http://arxiv.org/abs/astro-ph/0208231
Autor:
Ziegler, B. L., Boehm, A., Fricke, K. J., Jaeger, K., Nicklas, H., Bender, R., Drory, N., Gabasch, A., Saglia, R. P., Seitz, S., Heidt, J., Mehlert, D., Moellenhoff, C., Noll, S., Sutorius, E.
We present the B-band Tully-Fisher relation (TFR) of 60 late-type galaxies with redshifts 0.1-1. The galaxies were selected from the FORS Deep Field with a limiting magnitude of R=23. Spatially resolved rotation curves were derived from spectra obtai
Externí odkaz:
http://arxiv.org/abs/astro-ph/0111146
Autor:
Heidt, J., Appenzeller, I., Bender, R., Boehm, A., Drory, N., Fricke, K. J., Gabasch, A., Hopp, U., Jaeger, K., Kuemmel, M., Mehlert, D., Moellenhoff, C., Moorwood, A., Nicklas, H., Noll, S., Saglia, R., Seifert, W., Seitz, S., Stahl, O., Sutorius, E., Szeifert, T., Wagner, S. J., Ziegler, B.
Dedicating a major fraction of its guaranteed time, the FORS consortium established a FORS Deep Field which contains a known QSO at z = 3.36. It was imaged in UBgRIz with FORS at the VLT as well as in J and Ks with the NTT. Covering an area 6-8 times
Externí odkaz:
http://arxiv.org/abs/astro-ph/0101491
Publikováno v:
Astrophys.Space Sci. 276 (2001) 633-641
For the intermediate-type barred galaxy NGC2336 stationary models are constructed which reproduce in a consistent manner the observed distribution of the luminous matter and the observed gas kinematics in those regions affected by the bar. We present
Externí odkaz:
http://arxiv.org/abs/astro-ph/9902208