Zobrazeno 1 - 10
of 2 906
pro vyhledávání: '"Gómez, P. C."'
Autor:
Das, Swagat R., Merello, Manuel, Bronfman, Leonardo, Liu, Tie, Garay, Guido, Stutz, Amelia, Mardones, Diego, Zhou, Jian-Wen, Sanhueza, Patricio, Liu, Hong-Li, Vázquez-Semadeni, Enrique, Gómez, Gilberto C., Palau, Aina, Tej, Anandmayee, Xu, Feng-Wei, Baug, Tapas, Dewangan, Lokesh K., He, Jinhua, Zhu, Lei, Li1, Shanghuo, Juvela, Mika, Saha, Anindya, Issac, Namitha, Hwang, Jihye, Nazeer, Hafiz, Toth, L. Viktor
Hub-filament systems are considered as natural sites for high-mass star formation. Kinematic analysis of the surroundings of hub-filaments is essential to better understand high-mass star formation within such systems. In this work, we present a deta
Externí odkaz:
http://arxiv.org/abs/2409.19204
Autor:
Zamora-Aviles, Manuel, Camacho, Vianey, Ballesteros-Paredes, Javier, Vázquez-Semadeni, Enrique, Palau, Aina, Román-Zúñiga, Carlos, Hernández-Cruz, Andrés, Gómez, Gilberto C., Quesada-Zúñiga, Fabián, Naranjo-Romero, Raúl
We explore the Schmidt-Kennicutt (SK) relations and the star formation efficiency per free-fall time ($\eff$), mirroring observational studies, in numerical simulations of filamentary molecular clouds undergoing gravitational contraction. We find tha
Externí odkaz:
http://arxiv.org/abs/2409.11588
Autor:
Vázquez-Semadeni, Enrique, Palau, Aina, Gómez, Gilberto C., Arroyo-Chávez, Griselda, Alig, Christian, Ballesteros-Paredes, Javier, Camacho, Vianey, González-Samaniego, Alejandro, Burkert, Andreas
We provide a detailed comparison between the ``gravoturbulent'' (GT) and ``global hierarchical collapse'' (GHC) models for molecular clouds and star formation, their respective interpretations of the observational data, the features they share, and s
Externí odkaz:
http://arxiv.org/abs/2408.10406
We investigate the alignment mechanism between the magnetic field and interstellar clouds formed by the collision of warm atomic gas. We find that the magnetic field, initially oriented parallel to the flow, is perturbed by a fast MHD shock, which am
Externí odkaz:
http://arxiv.org/abs/2405.08702
Autor:
Mai, Xiaofeng, Liu, Tie, Liu, Xunchuan, Zhu, Lei, Garay, Guido, Goldsmith, Paul F., Juvela, Mika, Liu, Hongli, Mannfors, Emma, Tej, Anandmayee, Sanhueza, Patricio, Li, Shanghuo, Xu, Fengwei, Semadeni, Enrique Vazquez, Jiao, Wenyu, Peng, Yaping, Baug, T., Yang, Aiyuan, Dewangan, Lokesh, Bronfman, Leonardo, Gómez, Gilberto C., Palau, Aina, Lee, Chang Won, Qin, Sheng-Li, Tatematsu, Ken'ichi, Chibueze, James O., Yang, Dongting, Lu, Xing, Luo, Qiuyi, Gu, Qilao, Issac, Namitha, Zhang, Suinan, Li, Pak-Shing, Zhang, Bo, Tóth, L. Viktor
Only a handful of massive starless core candidates have been discovered so far, but none of them have been fully confirmed. Within the MM1 clump in the filamentary infrared dark cloud G34.43+0.24 that was covered by the ALMA-ATOMS survey at Band 3 ($
Externí odkaz:
http://arxiv.org/abs/2401.04322
Autor:
Blánquez-Sesé, David, Magdis, G. E., Gómez-Guijarro, C., Shuntov, M., Kokorev, V., Brammer, G., Valentino, F., Díaz-Santos, T., Paspaliaris, E. -D., Rigopoulou, D., Hjorth, J., Langeroodi, D., Gobat, R., Jin, S., Sillassen, N. B., Gillman, S., Greve, T. R., Lee, M.
Publikováno v:
A&A 679, L2 (2023)
We present a study of the mid-IR (MIR) emission of quiescent galaxies (QGs) beyond the local universe. Using deep $JWST$ imaging in the SMACS-0723 cluster field we identify a mass limited ($M_{*} >10^{9}$M$_{\odot}$) sample of intermediate redshift Q
Externí odkaz:
http://arxiv.org/abs/2310.01601
Autor:
Ciesla, L., Elbaz, D., Ilbert, O., Buat, V., Magnelli, B., Narayanan, D., Daddi, E., Gómez-Guijarro, C., Arango-Toro, R.
Publikováno v:
A&A 686, A128 (2024)
Star formation histories (SFH) of early (6$
Externí odkaz:
http://arxiv.org/abs/2309.15720
Autor:
Xu, Fengwei, Wang, Ke, Liu, Tie, Tang, Mengyao, Evans II, Neal J., Palau, Aina, Morii, Kaho, He, Jinhua, Sanhueza, Patricio, Liu, Hong-Li, Stutz, Amelia, Zhang, Qizhou, Chen, Xi, Li, Pak Shing, Gómez, Gilberto C., Vázquez-Semadeni, Enrique, Li, Shanghuo, Mai, Xiaofeng, Lu, Xing, Liu, Meizhu, Chen, Li, Li, Chuanshou, Shi, Hongqiong, Ren, Zhiyuan, Li, Di, Garay, Guido, Bronfman, Leonardo, Dewangan, Lokesh, Juvela, Mika, Lee, Chang Won, Zhang, S., Yue, Nannan, Wang, Chao, Ge, Yifei, Jiao, Wenyu, Luo, Qiuyi, Zhou, J. -W., Tatematsu, Ken'ichi, Chibueze, James O., Su, Keyun, Sun, Shenglan, Ristorcelli, I., Toth, L. Viktor
The ALMA Survey of Star Formation and Evolution in Massive Protoclusters with Blue Profiles (ASSEMBLE) aims to investigate the process of mass assembly and its connection to high-mass star formation theories in protoclusters in a dynamic view. We obs
Externí odkaz:
http://arxiv.org/abs/2309.14684
In many stochastic service systems, decision-makers find themselves making a sequence of decisions, with the number of decisions being unpredictable. To enhance these decisions, it is crucial to uncover the causal impact these decisions have through
Externí odkaz:
http://arxiv.org/abs/2307.07879
The formation mechanism of massive stars remains one of the main open problems in astrophysics, in particular the relationship between the mass of the most massive stars, and that of the cores in which they form. Numerical simulations of the formatio
Externí odkaz:
http://arxiv.org/abs/2306.13846