Zobrazeno 1 - 10
of 3 715
pro vyhledávání: '"Fisher, D. A."'
Autor:
Wang, Jing, Lin, Xuchen, Yang, Dong, Staveley-Smith, Lister, Walter, Fabian, Wang, Q. Daniel, Wang, Ran, Battisti, A. J., Catinella, Barbara, Chen, Hsiao-Wen, Cortese, Luca, Fisher, D. B., Ho, Luis C., Ji, Suoqing, Jiang, Peng, Kauffmann, Guinevere, Kong, Xu, Liu, Ziming, Shao, Li, Wang, Jie, Wang, Lile, Wang, Shun
We present a statistical study of the properties of diffuse HI in ten nearby galaxies, comparing the HI detected by the single-dish telescope FAST (FEASTS program) and the interferometer VLA (THINGS program), respectively. The THINGS' observation mis
Externí odkaz:
http://arxiv.org/abs/2404.09422
Autor:
Posses, A., Aravena, M., González-López, J., Schreiber, N. M. Förster, Liu, D., Lee, L., Solimano, M., Díaz-Santos, T., Assef, R. J., Barcos-Muñoz, L., Bovino, S., Bowler, R. A. A., Rivera, G. Calistro, da Cunha, E., Davies, R. L., Killi, M., De Looze, I., Ferrara, A., Fisher, D. B., Herrera-Camus, R., Ikeda, R., Lambert, T., Li, J., Lutz, D., Mitsuhashi, I., Palla, M., Relaño, M., Spilker, J., Naab, T., Tadaki, K., Telikova, K., Übler, H., van der Giessen, S., Villanueva, V.
The ALMA [CII] Resolved Ism in STar-forming gALaxies (CRISTAL) survey is a Cycle 8 ALMA Large Programme that studies the cold gas component of high-redshift galaxies. Its sub-arcsecond resolution observations are key to disentangling physical mechani
Externí odkaz:
http://arxiv.org/abs/2403.03379
Autor:
Solimano, M., González-López, J., Aravena, M., Herrera-Camus, R., De Looze, I., Schreiber, N. M. Förster, Spilker, J., Tadaki, K., Assef, R. J., Barcos-Muñoz, L., Davies, R. L., Díaz-Santos, T., Ferrara, A., Fisher, D. B., Guaita, L., Ikeda, R., Johnston, E. J., Lutz, D., Mitsuhashi, I., Moya-Sierralta, C., Relaño, M., Naab, T., Posses, A. C., Telikova, K., Übler, H., van der Giessen, S., Villanueva, V.
Massive star-forming galaxies in the high-redshift universe host large reservoirs of cold gas in their circumgalactic medium (CGM). Traditionally, these reservoirs have been linked to diffuse H I Lyman-$\alpha$ (Ly$\alpha)$ emission extending beyond
Externí odkaz:
http://arxiv.org/abs/2401.04919
Autor:
van de Sande, J., Fraser-McKelvie, A., Fisher, D. B., Martig, M., Hayden, M. R., collaboration, the GECKOS Survey
We present GECKOS (Generalising Edge-on galaxies and their Chemical bimodalities, Kinematics, and Outflows out to Solar environments), a new ESO VLT/MUSE large program. The main aim of GECKOS is to reveal the variation in key physical processes of di
Externí odkaz:
http://arxiv.org/abs/2306.00059
Autor:
Herrera-Camus, R., Schreiber, N. M. Förster, Price, S. H., Übler, H., Bolatto, A. D., Davies, R. L., Fisher, D., Genzel, R., Lutz, D., Naab, T., Nestor, A., Shimizu, T., Sternberg, A., Tacconi, L., Tadaki, K.
Publikováno v:
A&A 665, L8 (2022)
We present a kinematic analysis of the main-sequence galaxy HZ4 at $z=5.5$. Our study is based on deep, spatially resolved observations of the [CII] 158 $\mu$m transition obtained with the Atacama Large Millimeter/Submillimeter Array (ALMA). From the
Externí odkaz:
http://arxiv.org/abs/2203.00689
Autor:
Fisher, D. B., Bolatto, A. D., Glazebrook, K., Obreschkow, D., Obreschkow, R. G., Kacprzak, G. G., Nielsen, N. M.
We report on the internal distribution of star formation efficiency in IRAS 08339+6517 (hereafter IRAS08), using $\sim$200~pc resolution CO(2-1) observations from NOEMA. The molecular gas depletion time changes by 2 orders-of-magnitude from disk-like
Externí odkaz:
http://arxiv.org/abs/2202.00024
Autor:
Saho, E., Hindmarsh, S., Sanchez, A.M., Birks, F., Kermode, J.R., Dale, M.W., Fisher, D., Beanland, R.
Publikováno v:
In Diamond & Related Materials April 2024 144
Autor:
Herrera-Camus, R., Schreiber, N. Förster, Genzel, R., Tacconi, L., Bolatto, A., Davies, R. L., Fisher, D., Lutz, D., Naab, T., Shimizu, T., Tadaki, K., Übler, H.
Publikováno v:
A&A 649, A31 (2021)
We present new Atacama Large Millimeter/Submillimeter Array (ALMA) observations of the [CII] 158 $\mu$m transition and the dust continuum in HZ4, a typical star-forming galaxy when the Universe was only $\sim1$ Gyr old ($z\approx5.5$). Our high $\app
Externí odkaz:
http://arxiv.org/abs/2101.05279
Autor:
Girard, M., Fisher, D. B., Bolatto, A. D., Abraham, R., Bassett, R., Glazebrook, K., Herrera-Camus, R., Jiménez, E., Lenkić, L., Obreschkow, D.
We compare the molecular and ionized gas velocity dispersion of 9 nearby turbulent disks, analogues to high-redshift galaxies, from the DYNAMO sample using new ALMA and GMOS/Gemini observations. We combine our sample with 12 galaxies at $z\sim $0.5-2
Externí odkaz:
http://arxiv.org/abs/2101.04122
Autor:
Foster, C., Mendel, J. T., Lagos, C. D. P., Wisnioski, E., Yuan, T., D'Eugenio, F., Barone, T. M., Harborne, K. E., Vaughan, S. P., Schulze, F., Remus, R. -S., Gupta, A., Collacchioni, F., Khim, D. J., Taylor, P., Bassett, R., Croom, S. M., McDermid, R. M., Poci, A., Battisti, A. J., Bland-Hawthorn, J., Bellstedt, S., Colless, M., Davies, L. J. M., Derkenne, C., Driver, S., Ferré-Mateu, A., Fisher, D. B., Gjergo, E., Johnston, E. J., Khalid, A., Kobayashi, C., Oh, S., Peng, Y., Robotham, A. S. G., Sharda, P., Sweet, S. M., Taylor, E. N., Tran, K. -V. H., Trayford, J. W., van de Sande, J., Yi, S. K., Zanisi, L.
We present an overview of the Middle Ages Galaxy Properties with Integral Field Spectroscopy (MAGPI) survey, a Large Program on ESO/VLT. MAGPI is designed to study the physical drivers of galaxy transformation at a lookback time of 3-4 Gyr, during wh
Externí odkaz:
http://arxiv.org/abs/2011.13567