Zobrazeno 1 - 10
of 149
pro vyhledávání: '"Meurer, Gerhardt R."'
We present a multi-wavelength (from far ultraviolet to HI emission) study of star formation feedback on the kinematics of the interstellar medium in the Sculptor Galaxy, NGC253. Its three well-known features (a disrupted stellar disc, a previously re
Externí odkaz:
http://arxiv.org/abs/2306.06869
Autor:
Pirzkal, Norbert, Malhotra, Sangeeta, Ryan, Russell E., Rothberg, Barry, Grogin, Norman, Finkelstein, Steven L., Koekemoer, Anton M., Rhoads, James, Larson, Rebecca L., Christensen, Lise, Cimatti, Andrea, Ferreras, Ignacio, Gardner, Jonathan P., Gronwall, Caryl, Hathi, Nimish P., Hibon, Pascale, Joshi, Bhavin, Kuntschner, Harald, Meurer, Gerhardt R., O’Connell, Robert W., Oestlin, Goeran, Pasquali, Anna, Pharo, John, Straughn, Amber N., Walsh, Jeremy R., Watson, Darach, Windhorst, Rogier A., Zakamska, Nadia L, Zirm, Andrew
The Faint Infrared Grism Survey (FIGS) is a deep Hubble Space Telescope (HST) WFC3/IR (Wide Field Camera 3 Infrared) slitless spectroscopic survey of four deep fields. Two fields are located in the Great Observatories Origins Deep Survey-North (GOODS
Externí odkaz:
http://hdl.handle.net/10150/625750
http://arizona.openrepository.com/arizona/handle/10150/625750
http://arizona.openrepository.com/arizona/handle/10150/625750
Autor:
Kim, Shin-Jeong, Oh, Se-Heon, Wang, Jing, Staveley-Smith, Lister, Koribalski, Bärbel S., Kim, Minsu, Park, Hye-Jin, Kim, Shinna, Spekkens, Kristine, Westmeier, Tobias, Wong, O. Ivy, Meurer, Gerhardt R., Kamphuis., Peter, Catinella, Barbara, McQuinn, Kristen B. W., Bigiel, Frank, Holwerda, Benne W., Rhee, Jonghwan, Lee-Waddell, Karen, Deg, Nathan, Verdes-Montenegro, Lourdes, For, Bi-Qing, Madrid, Juan P., Dénes, Helga, Elagali, Ahmed
We examine the HI gas kinematics of galaxy pairs in two clusters and a group using Australian Square Kilometre Array Pathfinder (ASKAP) WALLABY pilot survey observations. We compare the HI properties of galaxy pair candidates in the Hydra I and Norma
Externí odkaz:
http://arxiv.org/abs/2211.15123
Autor:
Glowacki, Marcin, Collier, Jordan D., Kazemi-Moridani, Amir, Frank, Bradley, Roberts, Hayley, Darling, Jeremy, Klöckner, Hans-Rainer, Adams, Nathan, Baker, Andrew J., Bershady, Matthew, Blecher, Tariq, Blyth, Sarah-Louise, Bowler, Rebecca, Catinella, Barbara, Chemin, Laurent, Crawford, Steven M., Cress, Catherine, Davé, Romeel, Deane, Roger, de Blok, Erwin, Delhaize, Jacinta, Duncan, Kenneth, Elson, Ed, February, Sean, Gawiser, Eric, Hatfield, Peter, Healy, Julia, Henning, Patricia, Hess, Kelley M., Heywood, Ian, Holwerda, Benne W., Hoosain, Munira, Hughes, John P., Hutchens, Zackary L., Jarvis, Matt, Kannappan, Sheila, Katz, Neal, Kereš, Dušan, Korsaga, Marie, Kraan-Korteweg, Renée C., Lah, Philip, Lochner, Michelle, Maddox, Natasha, Makhathini, Sphesihle, Meurer, Gerhardt R., Meyer, Martin, Obreschkow, Danail, Oh, Se-Heon, Oosterloo, Tom, Oppor, Joshua, Pan, Hengxing, Pisano, D. J., Randriamiarinarivo, Nandrianina, Ravindranath, Swara, Schröder, Anja C., Skelton, Rosalind, Smirnov, Oleg, Smith, Mathew, Somerville, Rachel S., Srianand, Raghunathan, Staveley-Smith, Lister, Tanaka, Masayuki, Vaccari, Mattia, van Driel, Wim, Verheijen, Marc, Walter, Fabian, Wu, John F., Zwaan, Martin A.
In the local Universe, OH megamasers (OHMs) are detected almost exclusively in infrared-luminous galaxies, with a prevalence that increases with IR luminosity, suggesting that they trace gas-rich galaxy mergers. Given the proximity of the rest freque
Externí odkaz:
http://arxiv.org/abs/2204.02523
Autor:
Audcent-Ross, Fiona M., Meurer, Gerhardt R., Audcent, James R., Ryder, Stuart D., Wong, O. Ivy, Phan, J., Williamson, A., Kim, J. H.
Given the limited availability of direct evidence (pre-explosion observations) for supernova (SN) progenitors, the location of supernovae (SNe) within their host galaxies can be used to set limits on one of their most fundamental characteristics, the
Externí odkaz:
http://arxiv.org/abs/1911.09842
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:
Pirzkal, Norbert, Rothberg, Barry, Ryan, Russell E., Malhotra, Sangeeta, Rhoads, James, Grogin, Norman, Curtis-Lake, Emma, Chevallard, Jacopo, Charlot, Stephane, Finkelstein, Steven L., Koekemoer, Anton M., Ghavamian, Parviz, Rodrigues, Myriam, Hammer, François, Puech, Mathieu, Larson, Rebecca L., Christensen, Lise, Cimatti, Andrea, Ferreras, Ignacio, Gardner, Jonathan P., Gronwall, Caryl, Hathi, Nimish P., Joshi, Bhavin, Kuntschner, Harald, Meurer, Gerhardt R., O'Connell, Robert W., Oestlin, Goeran, Pasquali, Anna, Pharo, John, Straughn, Amber N., Walsh, Jeremy R., Watson, Darach, Windhorst, Rogier A., Zakamsk, Nadia L
We present the results from the application of a two-dimensional emission line detection method, EMission-line two-Dimensional (EM2D), to the near-infrared G102 grism observations obtained with the Wide-Field Camera 3 (WFC3) as part of the Cycle 22 {
Externí odkaz:
http://arxiv.org/abs/1806.01787
Autor:
Watts, Adam B., Meurer, Gerhardt R., Lagos, Claudia D. P., Bruzzese, Sarah M., Kroupa, Pavel, Jerabkova, Tereza
We present optical photometry of Hubble Space Telescope (HST) ACS/WFC data of the resolved stellar populations in the outer disc of the dwarf irregular galaxy DDO 154. The photometry reveals that young main sequence stars are almost absent from the o
Externí odkaz:
http://arxiv.org/abs/1804.07072
Autor:
Meurer, Gerhardt R., Obreschkow, Danail, Wong, O. Ivy, Zheng, Zheng, Audcent-Ross, Fiona M., Hanish, D. J.
Publikováno v:
2018, MNRAS, 476, 1624-1636
HI-Selected galaxies obey a linear relationship between their maximum detected radius Rmax and rotational velocity. This result covers measurements in the optical, ultraviolet, and HI emission in galaxies spanning a factor of 30 in size and velocity,
Externí odkaz:
http://arxiv.org/abs/1803.04716
Autor:
Bekki, Kenji, Meurer, Gerhardt R.
We investigate the time evolution and spatial variation of the stellar initial mass function (IMF) in star-forming disk galaxies by using chemodynamical simulations with an IMF model depending both on local densities and metallicities ([Fe/H]) of the
Externí odkaz:
http://arxiv.org/abs/1301.7128