Zobrazeno 1 - 10
of 379
pro vyhledávání: '"Fathi K"'
Autor:
Izumi, T., Kohno, K., Fathi, K., Hatziminaoglou, E., Davies, R. I., Martín, S., Matsushita, S., Schinnerer, E., Espada, D., Aalto, S., Onishi, K., Turner, J. L., Imanishi, M., Nakanishi, K., Meier, D. S., Wada, K., Kawakatu, N., Nakajima, T.
We used the Atacama Large Millimeter/submillimeter Array (ALMA) to map the CO(3-2) and the underlying continuum emissions around the type 1 low-luminosity active galactic nucleus (LLAGN; bolometric luminosity $\lesssim 10^{42}$ erg~s$^{-1}$) of NGC 1
Externí odkaz:
http://arxiv.org/abs/1707.05806
Autor:
Martin, S., Kohno, K., Izumi, T., Krips, M., Meier, D. S., Aladro, R., Matsushita, S., Takano, S., Turner, J. L., Espada, D., Nakajima, T., Terashima, Y., Fathi, K., Hsieh, P. -Y., Imanishi, M., Lundgren, A., Nakai, N., Schinnerer, E., Sheth, K., Wiklind, T.
Publikováno v:
A&A 573, A116 (2015)
The nearby Sy 1 galaxy NGC 1097 represents an ideal laboratory to explore the molecular chemistry in the presence and surroundings of an active galactic nucleus. Exploring the distribution of different molecular species allows us to understand the ph
Externí odkaz:
http://arxiv.org/abs/1410.2823
Autor:
Piñol-Ferrer, N., Fathi, K., Carignan, C., Font, J., Hernandez, O., Karlsson, R., van de Ven, G.
We present the first galactic-scale model of the gas dynamics of the prototype barred Seyfert 1 galaxy NGC1097. We use large scale FaNTOmM Fabry-Perot interferometric data covering the entire galactic disc and combine the distribution and kinematics
Externí odkaz:
http://arxiv.org/abs/1311.2953
Autor:
Sandberg, A., Östlin, G., Hayes, M., Fathi, K., Schaerer, D., Mas-Hesse, J. M., Rivera-Thorsen, T.
Context. The Lyman alpha emission line of galaxies is an important tool for finding galaxies at high redshift, and thus probe the structure of the early universe. However, the resonance nature of the line and its sensitivity to dust and neutral gas i
Externí odkaz:
http://arxiv.org/abs/1303.2011
Circumstellar debris disks older than a few Myr should be largely devoid of primordial gas remaining from the protoplanetary disk phase. Tracing the origin of observed atomic gas in Keplerian rotation in the edge-on debris disk surrounding the ~12 My
Externí odkaz:
http://arxiv.org/abs/1207.4427
A code, Epic5, has been developed which computes, in the two-dimensional case, the initially circular orbits of guiding centra in an arbitrary axisymmetric potential with an arbitrary, weak perturbing potential in solid body rotation. This perturbing
Externí odkaz:
http://arxiv.org/abs/1112.3658
We report new near-IR integral field spectroscopy of the central starburst region of the barred spiral galaxy M83 obtained with CIRPASS on Gemini-S, which we analyse in conjunction with GHaFaS Fabry-Perot data, an AAT IRIS2 Ks-band image, and near- a
Externí odkaz:
http://arxiv.org/abs/1006.2698
Autor:
Santander-García, M., Rodríguez-Gil, P., Hernandez, O., Corradi, R. L. M., Jones, D., Giammanco, C., Beckman, J. E., Carignan, C., Fathi, K., Rubio-Díez, M. M., Jiménez-Luján, F., Benn, C. R.
The link between the shaping of bipolar planetary nebulae and their central stars is still poorly understood. The kinematics and shaping of the multipolar nebula M 1-75 are hereby investigated, and the location and nature of its central star are brie
Externí odkaz:
http://arxiv.org/abs/1006.2398
Autor:
Hernandez, O., Fathi, K., Carignan, C., Beckman, J., Gach, J. -L., Balard, P., Amram, P., Boulesteix, J., Corradi, R. L. M., de Denus-Baillargeon, M-M., Epinat, B., Relaño, M., Thibault, S., Vallée, P.
GH$\alpha$FaS a new Fabry-Perot system, is now available at the William Herschel Telescope. It was mounted, for the first time, at the Nasmyth focus of the 4.2 meter WHT on La Palma in July 2007. Using modern technology, with a spectral resolution of
Externí odkaz:
http://arxiv.org/abs/0805.0168
Autor:
Dicaire, I., Carignan, C., Amram, P., Hernandez, O., Chemin, L., Daigle, O., de Denus-Baillargeon, M. -M., Balkowski, C., Boselli, A., Fathi, K., Kennicutt, R. C.
This is the second part of an H-alpha kinematics follow-up survey of the Spitzer Infrared Nearby Galaxies Survey (SINGS) sample. The aim of this program is to shed new light on the role of baryons and their kinematics and on the dark/luminous matter
Externí odkaz:
http://arxiv.org/abs/0801.2971