Zobrazeno 1 - 10
of 37
pro vyhledávání: '"Jachym, Pavel"'
Autor:
Hu, Dan, Zajaček, Michal, Werner, Norbert, Grossová, Romana, Jáchym, Pavel, Roberts, Ian D., Ignesti, Alessandro, Kenney, Jeffrey D. P., Plšek, Tomáš, Breuer, Jean-Paul, Shimwell, Timothy, Tasse, Cyril, Zhu, Zhenhao, Wu, Linhui
We report LOFAR and VLA detections of extended radio emission in the spiral galaxy HCG 97b, hosted by an X-ray bright galaxy group. The extended radio emission detected at 144 MHz, 1.4 GHz and 4.86 GHz is elongated along the optical disk and has a ta
Externí odkaz:
http://arxiv.org/abs/2304.13066
When galaxies move through the intracluster medium (ICM) inside galaxy clusters, the ram pressure of the ICM can strip the gas from galaxies. The stripped gas forms tails on the trailing side. These galaxies are hence dubbed ``jellyfish galaxies''. E
Externí odkaz:
http://arxiv.org/abs/2303.15500
Autor:
Waldron, William, Sun, Ming, Luo, Rongxin, Laudari, Sunil, Chatzikos, Marios, Sivanandam, Suresh, Kenney, Jeffrey D. P., Jachym, Pavel, Voit, G. Mark, Donahue, Megan, Fossati, Matteo
Publikováno v:
MNRAS 522 (2023) 173-194
We present the results from the HST WFC3 and ACS data on an archetypal galaxy undergoing ram pressure stripping (RPS), ESO 137-001, in the nearby cluster Abell 3627. ESO 137-001 is known to host a prominent stripped tail detected in many bands from X
Externí odkaz:
http://arxiv.org/abs/2302.07270
Autor:
Luo, Rongxin, Sun, Ming, Jáchym, Pavel, Waldron, Will, Fossati, Matteo, Fumagalli, Michele, Boselli, Alessandro, Combes, Francoise, Kenney, Jeffrey D. P., Li, Yuan, Gronke, Max
Ram pressure stripping (RPS) is an important process to affect the evolution of cluster galaxies and their surrounding environment. We present a large MUSE mosaic for ESO 137-001 and its stripped tails, and study the detailed distributions and kinema
Externí odkaz:
http://arxiv.org/abs/2212.03891
Autor:
Taylor, Rhys, Koppen, Joachim, Jachym, Pavel, Minchin, Robert, Palous, Jan, Rosenberg, Jessica, Schneider, Steven, Wunsch, Richard, Deshev, Boris
Using data from the Arecibo Galaxy Environment Survey, we report the discovery of five HI clouds in the Leo I group without detected optical counterparts. Three of the clouds are found midway between M96 and M95, one is only 10$^{\prime}$ from the so
Externí odkaz:
http://arxiv.org/abs/2209.10994
Autor:
Jáchym, Pavel, Sun, Ming, Yagi, Masafumi, Ge, Chong, Luo, Rongxin, Combes, Françoise, Kabátová, Anežka, Kenney, Jeffrey D. P., Scott, Tom C., Brinks, Elias
Publikováno v:
A&A 658, L5 (2022)
We report the detection of CO emission in the recently discovered multiphase isolated gas cloud in the nearby galaxy cluster Abell 1367. The cloud is located about 800 kpc in projection from the center of the cluster and at a projected distance of >
Externí odkaz:
http://arxiv.org/abs/2201.11141
Autor:
Laudari, Sunil, Jáchym, Pavel, Sun, Ming, Waldron, Will, Chatzikos, Marios, Kenney, Jeffrey, Luo, Rongxin, Nulsen, Paul, Sarazin, Craig, Combes, Françoise, Edge, Tim, Voit, G. Mark, Donahue, Megan, Cortese, Luca
Ram pressure stripping (RPS) is an important mechanism for galaxy evolution. In this work, we present results from HST and APEX observations of one RPS galaxy, ESO 137-002 in the closest rich cluster Abell 3627. The galaxy is known to host prominent
Externí odkaz:
http://arxiv.org/abs/2111.01821
Autor:
Ge, Chong, Sun, Ming, Yagi, Masafumi, Fossati, Matteo, Forman, William, Jáchym, Pavel, Churazov, Eugene, Zhuravleva, Irina, Boselli, Alessandro, Jones, Christine, Ji, Li, Luo, Rongxin
Galaxy clusters grow primarily through the continuous accretion of group-scale haloes. Group galaxies experience preprocessing during their journey into clusters. A star-bursting compact group, the Blue Infalling Group (BIG), is plunging into the nea
Externí odkaz:
http://arxiv.org/abs/2109.07964
Autor:
Cramer, William J., Kenney, Jeffrey D. P., Tonnesen, Stephanie, Smith, Rory, Wong, Tony, Jáchym, Pavel, Cortés, Juan R., Cortés, Paulo C., Wu, Yu-Ting
We investigate the effects of ram pressure on the molecular ISM in the disk of the Coma cluster galaxy NGC 4921, via high resolution CO observations. We present 6" resolution CARMA CO(1-0) observations of the full disk, and 0.4" resolution ALMA CO(2-
Externí odkaz:
http://arxiv.org/abs/2107.11731