Zobrazeno 1 - 10
of 90
pro vyhledávání: '"Kennicutt Jr., R."'
Autor:
Lamarche, C., Smith, J. D., Kreckel, K., Linden, S. T., Rogers, N. S. J., Skillman, E., Berg, D., Murphy, E., Pogge, R., Donnelly, G. P., Kennicutt Jr., R., Bolatto, A., Croxall, K., Groves, B., Ferkinhoff, C.
Accurately determining gas-phase metal-abundances within galaxies is critical as metals strongly affect the physics of the interstellar medium (ISM). To date, the vast majority of widely-used gas-phase abundance-indicators rely on emission from brigh
Externí odkaz:
http://arxiv.org/abs/2111.10385
Autor:
Linden, S. T., Murphy, E. J., Dong, D., Momjian, E., Kennicutt Jr., R. C., Meier, D. S., Schinnerer, E., Turner, J. L.
We present 3, 15, and 33 GHz imaging towards galaxy nuclei and extranuclear star-forming regions using the Karl G. Jansky Very Large Array as part of the Star Formation in Radio Survey. With $3-33$ GHz radio spectra, we measured the spectral indices
Externí odkaz:
http://arxiv.org/abs/2004.10230
Autor:
Audcent-Ross, Fiona M., Meurer, Gerhardt R., Wong, O. I., Zheng, Z., Hanish, D., Zwaan, M. A., Bland-Hawthorn, J., Elagali, A., Meyer, M., Putman, M. E., Ryan-Webber, E. V., Sweet, S. M., Thilker, D. A., Seibert, M., Allen, R., Dopita, M. A., Doyle-Pegg, M. T., Drinkwater, M., Ferguson, H. C., Freeman, K. C., Heckman, T. M., Kennicutt Jr, R. C., Kilborn, V. A., Kim, J. H., Knezek, P. M., Koribalski, B., Smith, R. C., Staveley-Smith, L., Webster, R. L., Werk, J. K.
For the first time both H$\alpha$ and far-ultraviolet (FUV) observations from an HI-selected sample are used to determine the dust-corrected star formation rate density (SFRD: $\dot{\rho}$) in the local Universe. Applying the two star formation rate
Externí odkaz:
http://arxiv.org/abs/1806.05875
Autor:
Murphy, E. J., Dong, D., Momjian, E., Linden, S., Kennicutt, Jr., R. C., Meier, D. S., Schinnerer, E., Turner, J. L.
We present 33 GHz imaging for 112 pointings towards galaxy nuclei and extranuclear star-forming regions at $\approx$2" resolution using the Karl G. Jansky Very Large Array (VLA) as part of the Star Formation in Radio Survey. A comparison with 33 GHz
Externí odkaz:
http://arxiv.org/abs/1711.03976
Autor:
Delgado, R. M. González, Fernandes, R. Cid, Pérez, E., García-Benito, R., Fernández, R. López, Lacerda, E. A. D., Cortijo-Ferrero, C., de Amorim, A. L., Asari, N. Vale, Sánchez, S. F., Walcher, C. J., Wisotzki, L., Mast, D., Alves, J., Ascasibar, Y., Bland-Hawthorn, J., Galbany, L., Kennicutt Jr., R. C., Márquez, I., Masegosa, J., Mollá, M., Sánchez-Blázquez, P., Vílchez, J. M., collaboration, CALIFA
The aim of this paper is to characterize the radial structure of the star formation rate (SFR) in galaxies in the nearby Universe as represented by the CALIFA survey. The sample under study contains 416 galaxies observed with IFS, covering a wide ran
Externí odkaz:
http://arxiv.org/abs/1603.00874
Autor:
van der Laan, T. P. R., Armus, L., Beirao, P., Sandstrom, K., Groves, B., Schinnerer, E., Draine, B. T., Smith, J. D., Galametz, M., Wolfire, M., Croxall, K., Dale, D., Camus, R. Herrera, Calzetti, D., Kennicutt Jr, R. C.
Publikováno v:
A&A 575, A83 (2015)
The manner in which gas accretes and orbits within circumnuclear rings has direct implications for the star formation process. In particular, gas may be compressed and shocked at the inflow points, resulting in bursts of star formation at these locat
Externí odkaz:
http://arxiv.org/abs/1501.07279
Autor:
García-Benito, R., Zibetti, S., Sánchez, S. F., Husemann, B., de Amorim, A. L., Castillo-Morales, A., Fernandes, R. Cid, Ellis, S. C ., Falcón-Barroso, J., Galbany, L., de Paz, A. Gil, Delgado, R. M. González, Lacerda, E. A. D., López-Fernandez, R., de Lorenzo-Cáceres, A., Lyubenova, M., Marino, R. A., Mast, D., Mendoza, M. A., Pérez, E., Asari, N. Vale, Aguerri, J. A. L., Ascasibar, Y., Bekeraitė, S., Bland-Hawthorn, J., Barrera-Ballesteros, J. K., Cano-Díaz, M., Catalán-Torrecilla, C., Cortijo, C., Delgado-Inglada, G., Demleitner, M., Dettmar, R. -J., Díaz, A. I., Florido, E., Gallazzi, A., García-Lorenzo, B., Gomes, J. M., Holmes, L., Iglesias-Páramo, J., Jahnke, K., Kalinova, V., Kehrig, C., Kennicutt Jr, R. C., López-Sánchez, Á. R., Márquez, I., Masegosa, J., Meidt, S. E., Mendez-Abreu, J., Mollá, M., Monreal-Ibero, A., Morisset, C., del Olmo, A., Papaderos, P., Pérez, I., Quirrenbach, A., Rosales-Ortega, F. F., Roth, M. M., Ruiz-Lara, T., Sánchez-Blázquez, P., Sánchez-Menguiano, L., Singh, R., Spekkens, K., Stanishev, V., Torres-Papaqui, J. P., van de Ven, G., Vilchez, J. M., Walcher, C. J., Wild, V., Wisotzki, L., Ziegler, B., Aceituno, J.
Publikováno v:
A&A 576, A135 (2015)
This paper describes the Second Public Data Release (DR2) of the Calar Alto Legacy Integral Field Area (CALIFA) survey. The data for 200 objects are made public, including the 100 galaxies of the First Public Data Release (DR1). Data were obtained wi
Externí odkaz:
http://arxiv.org/abs/1409.8302
Autor:
Delgado, R. M. González, Pérez, E., Fernandes, R. Cid, García-Benito, R., de Amorim, A. L., Sánchez, S. F., Husemann, B., Cortijo-Ferrero, C., Fernández, R. López, Sánchez-Blázquez, P., Bekeraite, S., Walcher, C. J., Falcón-Barroso, J., Gallazzi, A., van de Ven, G., Alves, J., Bland-Hawthorn, J., Kennicutt Jr., R. C., Kupko, D., Lyubenova, M., Mast, D., Mollá, M., Marino, R. A., Quirrenbach, A., Vílchez, J. M., Wisotzki, L., collaboration, CALIFA
We study the radial structure of the stellar mass surface density ($\mu$) and stellar population age as a function of the total stellar mass and morphology for a sample of 107 galaxies from the CALIFA survey. We use the fossil record to recover the s
Externí odkaz:
http://arxiv.org/abs/1310.5517
Autor:
CALIFA collaboration, Husemann, B., Jahnke, K., Sánchez, S. F., Barrado, D., Bekeraitė, S., Bomans, D. J., Castillo-Morales, A., Catalán-Torrecilla, C., Fernandes, R. Cid, Falcón-Barroso, J., García-Benito, R., Delgado, R. M. González, Iglesias-Páramo, J., Johnson, B. D., Kupko, D., López-Fernandez, R., Lyubenova, M., Marino, R. A., Mast, D., Miskolczi, A., Monreal-Ibero, A., de Paz, A. Gil, Pérez, E., Pérez, I., Rosales-Ortega, F. F., Ruiz-Lara, T., Schilling, U., van de Ven, G., Walcher, J., Alves, J., de Amorim, A. L., Backsmann, N., Barrera-Ballesteros, J. K., Bland-Hawthorn, J., Cortijo, C., Dettmar, R. -J., Demleitner, M., Díaz, A. I., Enke, H., Florido, E., Flores, H., Galbany, L., Gallazzi, A., García-Lorenzo, B., Gomes, J. M., Gruel, N., Haines, T., Holmes, L., Jungwiert, B., Kalinova, V., Kehrig, C., Kennicutt Jr, R. C., Klar, J., Lehnert, M. D., Lóez-Sáchez, Á. R., de Lorenzo-Cáceres, A., Mármol-Queraltó, E., Márquez, I., Mendez-Abreu, J., Mollá, M., del Olmo, A., Meidt, S. E., Papaderos, P., Puschnig, J., Quirrenbach, A., Roth, M. M., Sánchez-Blázquez, P., Spekkens, K., Singh, R., Stanishev, V., Trager, S. C., Vilchez, J. M., Wild, V., Wisotzki, L., Zibetti, S., Ziegler, B.
We present the first public data release of the CALIFA survey. It consists of science-grade optical datacubes for the first 100 of eventually 600 nearby (0.005
Externí odkaz:
http://arxiv.org/abs/1210.8150
Autor:
Botticella, M. T., Smartt, S. J., Kennicutt Jr., R. C., Cappellaro, E., Sereno, M., Lee, J. C.
The core collapse supernova (CCSN) rate provides a strong lower limit for the star formation rate (SFR). Progress in using it as a cosmic SFR tracer requires some confidence that it is consistent with more conventional SFR diagnostics in the nearby U
Externí odkaz:
http://arxiv.org/abs/1111.1692