Zobrazeno 1 - 10
of 281
pro vyhledávání: '"Brinks Elias"'
Publikováno v:
A&A 692, A51 (2024)
Optical observations of Blue Compact Dwarf galaxies (BCDs) show they typically have high specific star formation rates and low metallicites. A subset of these galaxies (those with the lowest gas phase metallicities) display cometary optical morpholog
Externí odkaz:
http://arxiv.org/abs/2410.21221
Autor:
García-Rodríguez Axel, Usero Antonio, García-Burillo Santiago, Bigiel Frank, Brinks Elias, Fuente Asunción, Leroy Adam K., Querejeta Miguel
Publikováno v:
EPJ Web of Conferences, Vol 265, p 00018 (2022)
The Taffy system stands out as one of the strongest gas-rich galaxy mergers with little star formation (SF) activity. We study the causes of this SF inefficiency by observing with the IRAM 30m telescope the line emission of several species in 6 posit
Externí odkaz:
https://doaj.org/article/5de063355e2d4c0abdaebf0edc343ee8
Autor:
Kovakkuni, Navyasree, Lelli, Federico, Duc, Pierre-alain, Boquien, Médéric, Braine, Jonathan, Brinks, Elias, Charmandaris, Vassilis, Combes, Francoise, Fensch, Jeremy, Lisenfeld, Ute, McGaugh, Stacy, Mihos, J. Chris, Pawlowski, Marcel. S., Revaz, Yves., Weilbacher, Peter. M.
Tidal dwarf galaxies (TDGs) are low-mass objects that form within tidal and/or collisional debris ejected from more massive interacting galaxies. We use CO($1-0$) observations from ALMA and integral-field spectroscopy from MUSE to study molecular and
Externí odkaz:
http://arxiv.org/abs/2309.06478
Publikováno v:
A&A 665, A155 (2022)
Many galaxy properties are known to correlate with the environment in which the galaxies are embedded. Their cold, neutral gas content, usually assessed through 21cm HI observations, is related to many other galaxy properties as it is the underlying
Externí odkaz:
http://arxiv.org/abs/2206.13533
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:
Cigan, Phil, Young, Lisa M., Gomez, Haley L., Madden, Suzanne C., De Vis, Pieter, Hunter, Deidre A., Elmegreen, Bruce G., Brinks, Elias
We present here far-infrared photometry of galaxies in a sample that is relatively unexplored at these wavelengths: low-metallicity dwarf galaxies with moderate star formation rates. Four dwarf irregular galaxies from the $\mathrm{L{\small{ITTLE}}}$
Externí odkaz:
http://arxiv.org/abs/2104.14599
Autor:
Chen, Hao, Sun, Ming, Yagi, Masafumi, Bravo-Alfaro, Hector, Brinks, Elias, Kenney, Jeffrey, Combes, Francoise, Sivanandam, Suresh, Jachym, Pavel, Fossati, Matteo, Gavazzi, Giuseppe, Boselli, Alessandro, Nulsen, Paul, Sarazin, Craig, Ge, Chong, Yoshida, Michitoshi, Roediger, Elke
Previous studies have revealed a population of galaxies in galaxy clusters with ram pressure stripped (RPS) tails of gas and embedded young stars. We observed 1.4 GHz continuum and HI emission with the Very Large Array in its B-configuration in two f
Externí odkaz:
http://arxiv.org/abs/2004.06743
Autor:
Kaufman, Michele, Elmegreen, Bruce G., Andersen, Morten, Elmegreen, Debra Meloy, Struck, Curtis, Bournaud, Frederic, Brinks, Elias, McGarry, James C.
New ALMA CO, HCO+, and 100 GHz continuum observations and Gemini NIFS K-band spectra are combined with previous radio to X-ray data to study Feature i, a highly luminous starburst clump on an outer arm of the interacting galaxy NGC 2207. This clump h
Externí odkaz:
http://arxiv.org/abs/2003.08827
Autor:
Jiang, Xue-Jian, Greve, Thomas R., Gao, Yu, Zhang, Zhi-Yu, Tan, Qinghua, de Grijs, Richard, Ho, Luis C., Michalowski, Michal J., Currie, Malcolm J., Wilson, Christine D., Brinks, Elias, Ao, Yiping, Zhao, Yinghe, He, Jinhua, Harada, Nanase, Yang, Chentao, Jiao, Qian, Chung, Aeree, Lee, Bumhyun, Smith, Matthew W. L., Liu, Daizhong, Matsushita, Satoki, Shi, Yong, Imanishi, Masatoshi, Rawlings, Mark G., Zhu, Ming, Eden, David, Davis, Timothy A., Li, Xiaohu
To study the high-transition dense-gas tracers and their relationships to the star formation of the inner $\sim$ 2 kpc circumnuclear region of NGC253, we present HCN $J=4-3$ and HCO$^+ J=4-3$ maps obtained with the James Clerk Maxwell Telescope (JCMT
Externí odkaz:
http://arxiv.org/abs/2003.06595
Autor:
Crocker, Alison F., Pellegrini, Eric, Smith, J. -D. T., Draine, Bruce T., Wilson, Christine D., Wolfire, Mark, Armus, Lee, Brinks, Elias, Dale, Daniel A., Groves, Brent, Herrera-Camus, Rodrigo, Hunt, Leslie K., Kennicutt, Robert C., Murphy, Eric J., Sandstrom, Karin, Schinnerer, Eva, Rigopoulou, Dimitra, Rosolowsky, Erik, van der Werf, Paul
Publikováno v:
The Astrophysical Journal 887 (2019) 105
We present resolved [CI] line intensities of 18 nearby galaxies observed with the SPIRE FTS spectrometer on the Herschel Space Observatory. We use these data along with resolved CO line intensities from $J_\mathrm{up} = 1$ to 7 to interpret what phas
Externí odkaz:
http://arxiv.org/abs/2001.05047