Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Ramos, A. Asensio"'
Autor:
Alonso-Herrero, A., Roche, P. F., Esquej, P., Gonzalez-Martin, O., Pereira-Santaella, M., Almeida, C. Ramos, Levenson, N. A., Packham, C., Ramos, A. Asensio, Mason, R. E., Espinosa, J. M. Rodriguez, Alvarez, C., Colina, L., Aretxaga, I., Diaz-Santos, T., Perlman, E., Telesco, C. M.
We present mid-infrared (MIR) 8-13micron spectroscopy of the nuclear regions of the interacting galaxy Arp299 (IC694+NGC3690) obtained with CanariCam (CC) on the 10.4m Gran Telescopio Canarias (GTC). The high angular resolution (~0.3-0.6arcsec) of th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bf999d9d57f1bce8636a3d2133b7ad5b
Double-peaked line profiles are commonly considered a hallmark of rotating disks, with the distance between the peaks a measure of the rotation velocity. However, double-peaks can arise also from radiative transfer effects in optically thick non-rota
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3356663e06ab3f6add1a8408061258e9
http://arxiv.org/abs/1202.1450
http://arxiv.org/abs/1202.1450
Autor:
Alonso-Herrero, Almudena, Almeida, Cristina Ramos, Mason, Rachel, Ramos, Andres Asensio, Roche, Patrick F., Levenson, Nancy A., Elitzur, Moshe, Packham, Christopher, Espinosa, Jose Miguel Rodriguez, Young, Stuart, Diaz-Santos, Tanio, Perez-Garcia, Ana M.
We used the CLUMPY torus models and a Bayesian approach to fit the infrared spectral energy distributions (SEDs) and ground-based high-angular resolution mid-infrared spectroscopy of 13 nearby Seyfert galaxies. This allowed us to put tight constraint
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::697b9f43e5e2410b8be8bfbaf068ec2f
http://arxiv.org/abs/1105.2368
http://arxiv.org/abs/1105.2368
Autor:
Almeida, C. Ramos, Sanchez-Portal, M., Perez-Garcia, A. M., Acosta-Pulido, J. A., Castillo, M., Ramos, A. Asensio, Gonzalez-Serrano, J. I., Alonso-Herrero, A., Espinosa, J. M. Rodriguez, Hatziminaoglou, E., Coia, D., Valtchanov, I., Povic, M., Esquej, P., Packham, C., Altieri, B.
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters 2011, 417, L46-L50
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC. Repositorio Institucional del CSIC
instname
We report far-infrared (FIR) imaging of the Seyfert 2 galaxy NGC 3081 in the range 70–500 μm, obtained with an unprecedented angular resolution, using the Herschel Space Observatory instruments PACS and SPIRE. The 11 kpc (∼70 arcsec) diameter st
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::131871bf0787d9fbc873ec61f1431de2
https://hdl.handle.net/10902/27025
https://hdl.handle.net/10902/27025
Autor:
Almeida, C. Ramos, Levenson, N. A., Alonso-Herrero, A., Ramos, A. Asensio, Espinosa, J. M. Rodriguez, Garcia, A. M. Perez, Packham, C., Mason, R., Radomski, J. T., Diaz-Santos, T.
We present new mid-infrared (MIR) imaging data for three Type-1 Seyfert galaxies obtained with T-ReCS on the Gemini-South Telescope at subarcsecond resolution. Our aim is to enlarge the sample studied in a previous work to compare the properties of T
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1945da96d7be0fe5b84adfbb82455e24