Zobrazeno 1 - 10
of 295
pro vyhledávání: '"Tonini, C."'
Autor:
Schaefer, A. L., Croom, S. M., Scott, N., Brough, S., Allen, J. T., Bekki, K., Bland-Hawthorn, J., Bloom, J. V., Bryant, J. J., Cortese, L., Davies, L. J. M., Federrath, C., Fogarty, L. M. R., Green, A. W., Groves, B., Hopkins, A. M., Konstantopoulos, I. S., López-Sánchez, A. R., Lawrence, J. S., McElroy, R. E., Medling, A. M., Owers, M. S., Pracy, M. B., Richards, S. N., Robotham, A. S. G., van de Sande, J., Tonini, C., Yi, S. K.
We explore the radial distribution of star formation in galaxies in the SAMI Galaxy Survey as a function of their local group environment. Using a sample of galaxies in groups (with halo masses less than $ \simeq 10^{14} \, \mathrm{M_{\odot}}$) from
Externí odkaz:
http://arxiv.org/abs/1811.11676
Autor:
Tiley, A. L., Bureau, M., Cortese, L., Harrison, C. M., Johnson, H. L., Stott, J. P., Swinbank, A. M., Smail, I., Sobral, D., Bunker, A. J., Glazebrook, K., Bower, R. G., Obreschkow, D., Bryant, J. J., Jarvis, M. J., Bland-Hawthorn, J., Magdis, G., Medling, A. M., Sweet, S. M., Tonini, C., Turner, O. J., Sharples, R. M., Croom, S. M., Goodwin, M., Konstantopoulos, I. S., Lorente, N. P. F., Lawrence, J. S., Mould, J., Owers, M. S., Richards, S. N.
We construct Tully-Fisher relations (TFRs), from large samples of galaxies with spatially-resolved H$\alpha$ emission maps from the K-band Multi-Object Spectrograph (KMOS) Redshift One Spectroscopic Survey (KROSS) at $z\approx1$. We compare these to
Externí odkaz:
http://arxiv.org/abs/1810.07202
Autor:
Bloom, J. V., Croom, S. M., Bryant, J. J., Schaefer, A. L., Bland-Hawthorn, J., Brough, S., Callingham, J., Cortese, L., Federrath, C., Scott, N., Van de Sande, J., D'Eugenio, F., Sweet, S., Tonini, C., Allen, J. T., Goodwin, M., Green, A. W., Konstantopoulos, I. S., Lawrence, J., Lorente, N., Medling, A. M., Owers, M. S., Richards, S. N., Sharp, R.
In order to determine the causes of kinematic asymmetry in the H$\alpha$ gas in the SAMI Galaxy Survey sample, we investigate the comparative influences of environment and intrinsic properties of galaxies on perturbation. We use spatially resolved H$
Externí odkaz:
http://arxiv.org/abs/1801.06628
Autor:
Bloom, J. V., Croom, S. M., Bryant, J. J., Callingham, J. R., Schaefer, A. L., Cortese, L., Hopkins, A. M., DEugenio, F., Scott, N., Glazebrook, K., Tonini, C., McElroy, R. E., Clark, H., Catinella, B., Allen, J. T., Bland-Hawthorn, J., Goodwin, M., Green, A. W., Konstantopoulos, I. S., Lawrence, J., Lorente, N., Medling, A. M., Owers, M. S., Richards, S. N., Sharp, R.
Publikováno v:
Monthly Notices of the Royal Astronomical Society 472.2 (2017): 1809-1824
We investigate the Tully-Fisher Relation (TFR) for a morphologically and kine- matically diverse sample of galaxies from the SAMI Galaxy Survey using 2 dimensional spatially resolved Halpha velocity maps and find a well defined relation across the st
Externí odkaz:
http://arxiv.org/abs/1711.10726
Autor:
Taranu, D. S., Obreschkow, D., Dubinski, J. J., Fogarty, L. M. R., van de Sande, J., Catinella, B., Cortese, L., Moffett, A., Robotham, A. S. G., Allen, J. T., Bland-Hawthorn, J., Bryant, J. J., Colless, M., Croom, S. M., D'Eugenio, F., Davies, R. L., Drinkwater, M. J., Driver, S. P., Goodwin, M., Konstantopoulos, I. S., Lawrence, J. S., López-Sánchez, Á. R., Lorente, N. P. F., Medling, A. M., Mould, J. R., Owers, M. S., Power, C., Richards, S. N., Tonini, C.
We introduce a method for modeling disk galaxies designed to take full advantage of data from integral field spectroscopy (IFS). The method fits equilibrium models to simultaneously reproduce the surface brightness, rotation and velocity dispersion p
Externí odkaz:
http://arxiv.org/abs/1710.03241
Autor:
Foster, C., van de Sande, J., D'Eugenio, F., Cortese, L., McDermid, R. M., Bland-Hawthorn, J., Brough, S., Bryant, J., Croom, S. M., Goodwin, M., Konstantopoulos, I. S., Lawrence, J., Lopez-Sanchez, A. R., Medling, A. M., Owers, M. S., Richards, S. N., Scott, N., Taranu, D. S., Tonini, C., Zafar, T.
Using the stellar kinematic maps and ancillary imaging data from the Sydney AAO Multi Integral field (SAMI) Galaxy Survey, the intrinsic shape of kinematically-selected samples of galaxies is inferred. We implement an efficient and optimised algorith
Externí odkaz:
http://arxiv.org/abs/1709.03585
Autor:
Tescari, E., Cortese, L., Power, C., Wyithe, J. S. B., Ho, I. -T., Crain, R. A., Bland-Hawthorn, J., Croom, S. M., Kewley, L. J., Schaye, J., Bower, R. G., Theuns, T., Schaller, M., Barnes, L., Brough, S., Bryant, J. J., Goodwin, M., Gunawardhana, M. L. P., Lawrence, J. S., Leslie, S. K., López-Sánchez, Á. R., Lorente, N. P. F., Medling, A. M., Richards, S. N., Sweet, S. M., Tonini, C.
This work presents a study of galactic outflows driven by stellar feedback. We extract main sequence disc galaxies with stellar mass $10^9\le$ M$_{\star}/$M$_{\odot} \le 5.7\times10^{10}$ at redshift $z=0$ from the highest resolution cosmological sim
Externí odkaz:
http://arxiv.org/abs/1709.01939
Autor:
Owers, M. S., Allen, J. T., Baldry, I., Bryant, J. J., Cecil, G. N., Cortese, L., Croom, S. M., Driver, S. P., Fogarty, L. M. R., Green, A. W., Helmich, E., de Jong, J. T. A., Kuijken, K., Mahajan, S., McFarland, J., Pracy, M. B., Robotham, A. G. S., Sikkema, G., Sweet, S., Taylor, E. N., Kleijn, G. Verdoes, Bauer, A. E., Bland-Hawthorn, J., Brough, S., Colless, M., Couch, W. J., Davies, R. L, Drinkwater, M. J., Goodwin, M., Hopkins, A. M., Konstantopoulos, I. S., Foster, C., Lawrence, J. S., Lorente, N. P. F, Medling, A. M., Metcalfe, N., Richards, S. N., van de Sande, J., Scott, N., Shanks, T., Sharp, R., Thomas, A. D., Tonini, C.
We describe the selection of galaxies targeted in eight low redshift clusters (APMCC0917, A168, A4038, EDCC442, A3880, A2399, A119 and A85; $0.029 < z < 0.058$) as part of the Sydney-AAO Multi-Object integral field Spectrograph Galaxy Survey (SAMI-GS
Externí odkaz:
http://arxiv.org/abs/1703.00997
Autor:
Cortese, L., Fogarty, L. M. R., Bekki, K., van de Sande, J., Couch, W., Catinella, B., Colless, M., Obreschkow, D., Taranu, D., Tescari, E., Barat, D., Bland-Hawthorn, J., Bloom, J., Bryant, J. J., Cluver, M., Croom, S. M., Drinkwater, M. J., d'Eugenio, F., Konstantopoulos, I. S., Lopez-Sanchez, A., Mahajan, S., Scott, N., Tonini, C., Wong, O. I., Allen, J. T., Brough, S., Goodwin, M., Green, A. W., Ho, I. -T., Kelvin, L. S., Lawrence, J. S., Lorente, N. P. F., Medling, A. M., Owers, M. S., Richards, S., Sharp, R., Sweet, S. M.
We investigate the relationship between stellar and gas specific angular momentum $j$, stellar mass $M_{*}$ and optical morphology for a sample of 488 galaxies extracted from the SAMI Galaxy Survey. We find that $j$, measured within one effective rad
Externí odkaz:
http://arxiv.org/abs/1608.00291
Intensity mapping of the neutral hydrogen (HI) is a new observational tool that can be used to efficiently map the large-scale structure of the Universe over wide redshift ranges. The power spectrum of the intensity maps contains cosmological informa
Externí odkaz:
http://arxiv.org/abs/1512.04189