Zobrazeno 1 - 10
of 147
pro vyhledávání: '"Michalowski, Michal~J."'
Autor:
Ryzhov, Oleh, Michałowski, Michał J., Nadolny, J., Hjorth, J., Leśniewska, A., Solar, M., Nowaczyk, P., Gall, C., Takeuchi, T. T.
Quenching of star-formation plays a fundamental role in galaxy evolution. This process occurs due to the removal of the cold interstellar medium (ISM) or stabilization against collapse, so that gas cannot be used in the formation of new stars. In thi
Externí odkaz:
http://arxiv.org/abs/2411.10517
Autor:
Solar, Martín, Michałowski, Michał J., Nadolny, Jakub, Galbany, Lluís, Hjorth, Jens, Zapartas, Emmanouil, Sollerman, Jesper, Hunt, Leslie, Klose, Sylvio, Koprowski, Maciej, Leśniewska, Aleksandra, Małkowski, Michał, Guelbenzu, Ana M. Nicuesa, Ryzhov, Oleh, Savaglio, Sandra, Schady, Patricia, Schulze, Steve, Postigo, Antonio de Ugarte, Vergani, Susanna D., Watson, Darach, Wróblewski, Radosław
Publikováno v:
Nat Commun 15, 7667 (2024)
Core-collapse supernovae are explosions of massive stars at the end of their evolution. They are responsible for metal production and for halting star formation, having a significant impact on galaxy evolution. The details of these processes depend o
Externí odkaz:
http://arxiv.org/abs/2409.01906
Autor:
Nadolny, Jakub, Michałowski, Michał J., Parente, Massimiliano, Hjorth, Jens, Gall, Christa, Leśniewska, Aleksandra, Solar, Martín, Nowaczyk, Przemysław, Ryzhov, Oleh
Publikováno v:
A&A 689, A210 (2024)
Removing cold interstellar medium (ISM) from a galaxy is central to quenching star formation. However, the exact mechanism of this process remains unclear. The objective of this work is to find the mechanism responsible for dust and gas removal in si
Externí odkaz:
http://arxiv.org/abs/2406.16533
Autor:
Michałowski, Michał J., Gall, C., Hjorth, J., Frayer, D. T., Tsai, A. -L., Rowlands, K., Takeuchi, T. T., Leśniewska, A., Behrendt, D., Bourne, N., Hughes, D. H., Koprowski, M. P., Nadolny, J., Ryzhov, O., Solar, M., Spring, E., Zavala, J., Bartczak, P.
Publikováno v:
2024, ApJ, 964, 129
Understanding how galaxies quench their star formation is crucial for studies of galaxy evolution. Quenching is related to the cold gas decrease. In the first paper we showed that the dust removal timescale in early-type galaxies (ETGs) is about 2.5
Externí odkaz:
http://arxiv.org/abs/2401.04774
Autor:
Nanni, Ambra, Cristallo, Sergio, Donevski, Darko, Michałowski, Michał J., Romano, Michael, Sawant, Prasad
Aims. We investigate the role of photo-evaporation of dust exposed to the radiation field from hot young stars and planetary nebulae (PNe) as a possible destruction mechanism of dust grains in the interstellar medium (ISM). Methods. We estimate photo
Externí odkaz:
http://arxiv.org/abs/2312.15998
Autor:
Smith, Matthew W. L., Eales, Stephen A., Williams, Thomas G., Lee, Bumhyun, Li, Zongnan, Barmby, Pauline, Bureau, Martin, Chapman, Scott, Cho, Brian S., Chung, Aeree, Chung, Eun Jung, Chung, Hui-Hsuan, Clark, Christopher J. R., Clements, David L., Davis, Timothy A., De Looze, Ilse, Eden, David J., Athikkat-Eknath, Gayathri, Ford, George P., Gao, Yu, Gear, Walter, Gomez, Haley L., de Grijs, Richard, He, Jinhua, Ho, Luis C., Hughes, Thomas M., Jiao, Sihan, Li, Zhiyuan, Kemper, Francisca, Kirchschlager, Florian, Koch, Eric W., Kong, Albert K. H., Lee, Chien-Hsiu, Lin, En-Tzu, Mairs, Steve, Michalowski, Michal J., Pattle, Kate, Peng, Yingjie, Ragan, Sarah E., Rawlings, Mark G., Rigopoulou, Dimitra, Saintonge, Amelie, Schruba, Andreas, Tang, Xindi, Wang, Junfeng, Whitworth, Anthony P., Wilson, Christine D., Yim, Kijeong, Zhu, Ming
Observing nearby galaxies with submillimeter telescopes on the ground has two major challenges. First, the brightness is significantly reduced at long submillimeter wavelengths compared to the brightness at the peak of the dust emission. Second, it i
Externí odkaz:
http://arxiv.org/abs/2110.00011
Autor:
Michałowski, Michał J.
Fast radio bursts (FRBs) are enigmatic transients with very short radio emission. Their nature is still widely debated. I provide the first analysis of atomic gas properties of a small sample of FRB hosts to constrain their nature. HI observations ex
Externí odkaz:
http://arxiv.org/abs/2109.02663
Autor:
Michałowski, Michał J., Mróz, Przemek
Gravitational lensing is an important prediction of general relativity, providing both its test and a tool to detect faint but amplified sources and to measure masses of lenses. For some applications (e.g. testing the theory), a point source lensed b
Externí odkaz:
http://arxiv.org/abs/2107.00659
Autor:
Pennock, Clara M., van Loon, Jacco Th., Filipovic, Miroslav D., Andernach, Heinz, Haberl, Frank, Kothes, Roland, Lenc, Emil, Rudnick, Lawrence, White, Sarah V., Agliozzo, Claudia, Antón, Sonia, Bojicic, Ivan, Bomans, Dominik J., Collier, Jordan D., Crawford, Evan J., Hopkins, Andrew M., Jeganathan, Kanapathippillai, Kavanagh, Patrick J., Koribalski, Bärbel S., Leahy, Denis, Maggi, Pierre, Maitra, Chandreyee, Marvil, Josh, Michałowski, Michał J., Norris, Ray P., Oliveira, Joana M., Payne, Jeffrey L., Sano, Hidetoshi, Sasaki, Manami, Staveley-Smith, Lister, Vardoulaki, Eleni
We present an analysis of a new 120 deg$^{2}$ radio continuum image of the Large Magellanic Cloud (LMC) at 888 MHz with a bandwidth of 288 MHz and beam size of $13\rlap{.}^{\prime\prime}9\times12\rlap{.}^{\prime\prime}1$, from the Australian Square K
Externí odkaz:
http://arxiv.org/abs/2106.12013
Autor:
Butler, Kirsty M., van der Werf, Paul P., Rybak, Matus, Costa, Tiago, Cox, Pierre, Weiß, Axel, Michałowski, Michał J., Riechers, Dominik A., Rigopoulou, Dimitra, Marchetti, Lucia, Eales, Stephen, Valtchanov, Ivan
We report the detection of a massive neutral gas outflow in the z=2.09 gravitationally lensed Dusty Star-Forming Galaxy HATLASJ085358.9+015537 (G09v1.40), seen in absorption with the OH+(1_1-1_0) transition using spatially resolved (0.5"x0.4") Atacam
Externí odkaz:
http://arxiv.org/abs/2104.10077