Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Bloom, Jessica V."'
Autor:
Medling, Anne M., Cortese, Luca, Croom, Scott M., Green, Andrew W., Groves, Brent, Hampton, Elise, Ho, I-Ting, Davies, Luke J. M., Kewley, Lisa J., Moffett, Amanda J., Schaefer, Adam L., Taylor, Edward, Zafar, Tayyaba, Bekki, Kenji, Bland-Hawthorn, Joss, Bloom, Jessica V., Brough, Sarah, Bryant, Julia J., Catinella, Barbara, Cecil, Gerald, Colless, Matthew, Couch, Warrick J., Drinkwater, Michael J., Driver, Simon P., Federrath, Christoph, Foster, Caroline, Goldstein, Gregory, Goodwin, Michael, Hopkins, Andrew, Lawrence, J. S., Leslie, Sarah K., Lewis, Geraint F., Lorente, Nuria P. F., Owers, Matt S., McDermid, Richard, Richards, Samuel N., Sharp, Robert, Scott, Nicholas, Sweet, Sarah M., Taranu, Dan S., Tescari, Edoardo, Tonini, Chiara, van de Sande, Jesse, Walcher, C. Jakob, Wright, Angus
We present the ~800 star formation rate maps for the SAMI Galaxy Survey based on H{\alpha} emission maps, corrected for dust attenuation via the Balmer decrement, that are included in the SAMI Public Data Release 1. We mask out spaxels contaminated b
Externí odkaz:
http://arxiv.org/abs/1801.04283
Autor:
Oh, Sree, Yi, Sukyoung K., Cortese, Luca, van de Sande, Jesse, Mahajan, Smriti, Jeong, Hyunjin, Sheen, Yun-Kyeong, Allen, James T., Bekki, Kenji, Bland-Hawthorn, Joss, Bloom, Jessica V., Brough, Sarah, Bryant, Julia J., Colless, Matthew, Croom, Scott M., Fogarty, L. M. R., Goodwin, Michael, Green, Andy, Konstantopoulos, Iraklis S., Lawrence, Jon, López-Sánchez, Á. R., Lorente, Nuria P. F., Medling, Anne M., Owers, Matt S., Richards, Samuel, Scott, Nicholas, Sharp, Rob, Sweet, Sarah M.
Galaxy mergers are important events that can determine the fate of a galaxy by changing its morphology, star-formation activity and mass growth. Merger systems have commonly been identified from their disturbed morphologies, and we now can employ Int
Externí odkaz:
http://arxiv.org/abs/1609.03595
Autor:
Ho, I-Ting, Kewley, Lisa J., Dopita, Michael A., Medling, Anne M., Allen, J. T., Bland-Hawthorn, Joss, Bloom, Jessica V., Bryant, Julia J., Croom, Scott M., Fogarty, L. M. R., Goodwin, Michael, Green, Andy W., Konstantopoulos, Iraklis S., Lawrence, Jon S., López-Sánchez, Á. R., Owers, Matt S., Richards, Samuel, Sharp, Rob
We demonstrate the feasibility and potential of using large integral field spectroscopic surveys to investigate the prevalence of galactic-scale outflows in the local Universe. Using integral field data from SAMI and the Wide Field Spectrograph, we s
Externí odkaz:
http://arxiv.org/abs/1407.2411