Zobrazeno 1 - 10
of 734
pro vyhledávání: '"Slater, R. A."'
Autor:
Kianfar, K., Andreani, P., Fernández-Ontiveros, J. A., Combes, F., Spinoglio, L., Hatziminaoglou, E., Ricci, C., Bewketu-Belete, A., Imanishi, M., Pereira-Santaella, M., Slater, R., Malheiro, M.
We investigate active galactic nuclei (AGN) feeding through the molecular gas (CO(2-1) emission) properties of the local Seyfert 1 galaxy NGC 4593, using Atacama Large Millimeter Array (ALMA) observations and other multi-wavelength data. Our study ai
Externí odkaz:
http://arxiv.org/abs/2410.09941
Autor:
Baldwin D, Carmichael J, Cook G, Navani N, Peach J, Slater R, Wheatstone P, Wilkins J, Allen-Delingpole N, Kerr CEP, Siddiqui K
Publikováno v:
Cancer Management and Research, Vol Volume 16, Pp 791-810 (2024)
David Baldwin,1 Jonathan Carmichael,2 Gordon Cook,3 Neal Navani,4,5 James Peach,6 Ruth Slater,7 Pete Wheatstone,8 Julia Wilkins,7 Nicola Allen-Delingpole,9 Cicely EP Kerr,10 Khalid Siddiqui11 1Department of Respiratory Medicine, Nottingham University
Externí odkaz:
https://doaj.org/article/6b69277b11ff456e9069da3babd8c4e3
Autor:
Belete, A. Bewketu, Andreani, P., Fernández-Ontiveros, J. A., Hatziminaoglou, E., Combes, F., Sirressi, M., Slater, R., Ricci, C., Dasyra, K., Cicone, C., Aalto, S., Spinoglio, L., Imanishi, M., De Medeiros, J. R.
Publikováno v:
A&A 654, A24 (2021)
We present the analysis of the molecular gas in the nuclear regions of NGC 4968, NGC 4845, and MCG-06-30-15, with the help of ALMA observations of the CO(2-1) emission line. The aim is to determine the kinematics of the gas in the central (~ 1 kpc) r
Externí odkaz:
http://arxiv.org/abs/2105.06867
Autor:
Fernández-Ontiveros, J. A., Dasyra, K. M., Hatziminaoglou, E., Malkan, M. A., Pereira-Santaella, M., Papachristou, M., Spinoglio, L., Combes, F., Aalto, S., Nagar, N., Imanishi, M., Andreani, P., Ricci, C., Slater, R.
Publikováno v:
A&A 633, A127 (2020)
A prominent jet-driven outflow of CO(2-1) molecular gas is found along the kinematic minor axis of the Seyfert 2 galaxy ESO 420-G13, at a distance of $340-600\, \rm{pc}$ from the nucleus. The wind morphology resembles a characteristic funnel shape, f
Externí odkaz:
http://arxiv.org/abs/1911.00015
Autor:
Ramakrishnan, V., Nagar, N. M., Finlez, C., Storchi-Bergmann, T., Slater, R., Schnorr-Müller, A., Riffel, R. A., Mundell, C. G., Robinson, A.
We present the molecular gas morphology and kinematics of seven nearby Seyfert galaxies obtained from our 230~GHz ALMA observations. The CO J=2-1 kinematics within the inner $\sim30$" ($\lesssim9$~kpc) reveals rotation patterns that have been explore
Externí odkaz:
http://arxiv.org/abs/1905.00994
Autor:
Slater, R., Finlez, C., Nagar, N. M., Schnorr-Müller, A., Storchi-Bergmann, T., Lena, D., Ramakrishnan, V., Mundell, C. G., Riffel, R. A., Peterson, B., Robinson, A., Orellana, G.
Publikováno v:
A&A 621, A83 (2019)
We aim to map the distribution and kinematics of molecular and ionized gas in a sample of active galaxies, to quantify the nuclear inflows and outflows. Here, we analyze the nuclear kinematics of NGC 1566 via ALMA observations of the CO J:2-1 emissio
Externí odkaz:
http://arxiv.org/abs/1804.02054
Autor:
Orellana, G., Elbaz, N. M. Nagar D., Calderón-Castillo, P., Leiton, R., Ibar, E., Magnelli, B., Daddi, E., Messias, H., Cerulo, P., Slater, R.
Publikováno v:
A&A 602, A68 (2017)
We aim to characterize the relationship between dust properties. We also aim to provide equations to estimate accurate dust properties from limited observational datasets. We assemble a sample of 1,630 nearby (z<0.1) galaxies-over a large range of Ms
Externí odkaz:
http://arxiv.org/abs/1703.09829
Autor:
Rodgers, K. B., Ishii, M., Frölicher, T. L., Schlunegger, S., Aumont, O., Toyama, K., Slater, R. D.
Publikováno v:
Journal of Climate, 2020 Dec 01. 33(23), 10321-10338.
Externí odkaz:
https://www.jstor.org/stable/27076094
Stars form with a complex and highly structured distribution. For a smooth star cluster to form from these initial conditions, the star cluster must erase this substructure. We study how substructure is removed using N-body simulations that realistic
Externí odkaz:
http://arxiv.org/abs/1105.1953
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