Zobrazeno 1 - 10
of 36
pro vyhledávání: '"Healy, Julia"'
Autor:
Eibensteiner, Cosima, Sun, Jiayi, Bigiel, Frank, Leroy, Adam K., Schinnerer, Eva, Rosolowsky, Erik, Kurapati, Sushma, Pisano, D. J., de Blok, W. J. G, Barnes, Ashley T., Thorp, Mallory, Colombo, Dario, Koch, Eric W., Chiang, I-Da, Ostriker, Eve C., Murphy, Eric J., Zabel, Nikki, Laudage, Sebstian, Maccagni, Filippo M., Healy, Julia, Sekhar, Srikrishna, Utomo, Dyas, Brok, Jakob den, Cao, Yixian, Chevance, Mélanie, Dale, Daniel A., Faesi, Christopher M., Glover, Simon C. O., He, Hao, Jeffreson, Sarah, Jiménez-Donaire, María J., Klessen, Ralf, Neumann, Justus, Pan, Hsi-An, Pathak, Debosmita, Querejeta, Miguel, Teng, Yu-Hsuan, Usero, Antonio, Williams, Thomas G.
The molecular-to-atomic gas ratio is crucial to the evolution of the interstellar medium in galaxies. We investigate the balance between the atomic ($\Sigma_{\rm HI}$) and molecular gas ($\Sigma_{\rm H2}$) surface densities in eight nearby star-formi
Externí odkaz:
http://arxiv.org/abs/2407.01716
Autor:
Deb, Tirna, Verheijen, Marc A. W., Poggianti, Bianca M., Moretti, Alessia, van der Hulst, J. M., Vulcani, Benedetta, Ramatsoku, Mpati, Serra, Paolo, Healy, Julia, Gullieuszik, Marco, Bacchini, Cecilia, Ignesti, Alessandro, Müller, Ancla, Zabel, Nikki, Luber, Nicholas, Jaffé, Yara L., Gitti, Myriam
We present MeerKAT HI observations of six jellyfish candidate galaxies (JFCGs) in the galaxy cluster, A2626. Two of the six galaxies JW100 and JW103, that were identified as JFCGs from B-band images, are confirmed as jellyfish galaxies (JFGs). Both o
Externí odkaz:
http://arxiv.org/abs/2208.12950
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:
Healy, Julia Lynn
The environment in which a galaxy resides has long been known to have an impact on how the galaxy evolves. The denser the environment, the stronger the influence. Clusters of galaxies, which are some of the densest known cosmic environments, provide
Externí odkaz:
http://hdl.handle.net/11427/35594
Autor:
Ignesti, Alessandro, Vulcani, Benedetta, Poggianti, Bianca M., Paladino, Rosita, Shimwell, Timothy, Healy, Julia, Gitti, Myriam, Bacchini, Cecilia, Moretti, Alessia, Radovich, Mario, van Weeren, Reinout J., Roberts, Ian D., Botteon, Andrea, Müller, Ancla, McGee, Sean, Fritz, Jacopo, Tomčić, Neven, Werle, Ariel, Mingozzi, Matilde, Gullieuszik, Marco, Verheijen, Marc
Ram pressure stripping is a crucial evolutionary driver for cluster galaxies. It is thought to be able to accelerate the evolution of their star formation, trigger the activity of their central active galactic nucleus (AGN) and the interplay between
Externí odkaz:
http://arxiv.org/abs/2110.12719
Autor:
Oman, Kyle A., Bahé, Yannick M., Healy, Julia, Hess, Kelley M., Hudson, Michael J., Verheijen, Marc A. W.
We combine orbital information from N-body simulations with an analytic model for star formation quenching and SDSS observations to infer the differential effect of the group/cluster environment on star formation in satellite galaxies. We also consid
Externí odkaz:
http://arxiv.org/abs/2009.00667
Autor:
Healy, Julia L
Neutral atomic hydrogen (Hi) is the raw fuel from which the star-forming molecular gas forms and is therefore an important tracer of galaxy evolution. Due to the intrinsic faintness of the Hi emission line (observed at rest at 21 cm), galaxies beyond
Externí odkaz:
http://hdl.handle.net/11427/24463
Autor:
Healy, Julia Lynn
The environment in which a galaxy resides has long been known to have an impact on how the galaxy evolves. The denser the environment, the stronger the influence. Clusters of galaxies, which are some of the densest known cosmic environments, provide
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3158::58bc56f7f076bccb6492637f3d64959c
http://hdl.handle.net/11427/35594
http://hdl.handle.net/11427/35594
Coherent horizontal stripe artefacts caused by low-level RFI coherently adding at the u=0 coordinate on the short baselines are visible in data cubes of deep radio interferometric observations. This affects the characterisation of low-intensity spect
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d26623e9c73fd099e6a81cb35c5dd1ad
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