Zobrazeno 1 - 10
of 53
pro vyhledávání: '"Luo, Rongxin"'
The luminosity and spectral energy distribution (SED) of high-$z$ galaxies are sensitive to the stellar population synthesis (SPS) models. In this paper, we study the effects of different SPS models on the measurements of high-$z$ galaxies and the bu
Externí odkaz:
http://arxiv.org/abs/2405.01821
Autor:
Kim, Changseok, Woo, Jong-Hak, Luo, Rongxin, Chung, Aeree, Baek, Junhyun, Le, Huynh Anh N., Son, Donghoon
We present spatially resolved gas kinematics, ionization, and energetics of 11 type 1 and 5 type 2 active galactic nuclei (AGNs) with strong ionized gas outflows at z $<0.3$ using Gemini Multi-Object Spectrograph Integral Field Unit (GMOS-IFU) data.
Externí odkaz:
http://arxiv.org/abs/2310.06928
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:
Kim, Changseok, Woo, Jong-Hak, Jadhav, Yashashree, Chung, Aeree, Baek, Junhyun, Lee, Jeong Ae, Shin, Jaejin, Hwang, Ho Seong, Luo, Rongxin, Son, Donghoon, Kim, HyunGi, Woo, Hyuk
We present the star formation rate (SFR) measurements based on the spectral energy distribution (SED) analysis with new sub-mm fluxes combined with archival multi-wavelength data for a sample of 52 AGN host galaxies at z $<0.2$. We carried out sub-mm
Externí odkaz:
http://arxiv.org/abs/2202.10044
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:
Ge, Chong, Luo, Rongxin, Sun, Ming, Yagi, Masafumi, Jáchym, Pavel, Boselli, Alessandro, Fossati, Matteo, Nulsen, Paul E. J., Sarazin, Craig, Edge, Tim, Gavazzi, Giuseppe, Gaspari, Massimo, Koda, Jin, Komiyama, Yutaka, Yoshida, Michitoshi
Recent studies have highlighted the potential significance of intracluster medium (ICM) clumping and its important implications for cluster cosmology and baryon physics. Many of the ICM clumps can originate from infalling galaxies, as stripped inters
Externí odkaz:
http://arxiv.org/abs/2104.03993