Zobrazeno 1 - 10
of 292
pro vyhledávání: '"Gronke, Max"'
Autor:
Li, Zhihui, Gronke, Max, Heckman, Timothy, Xu, Xinfeng, Henry, Alaina, Carr, Cody, Chisholm, John, Borthakur, Sanchayeeta, Marques-Chaves, Rui, Schaerer, Daniel, Leclercq, Floriane, Berg, Danielle A.
We conducted systematic radiative transfer (RT) modeling of the Mg II doublet line profiles for 33 low-redshift Lyman continuum (LyC) leakers, and Ly$\alpha$ modeling for a subset of six objects, using a multiphase, clumpy circumgalactic medium (CGM)
Externí odkaz:
http://arxiv.org/abs/2410.11152
Autor:
Solhaug, Erik, Chen, Hsiao-Wen, Chen, Mandy C., Zahedy, Fakhri, Gronke, Max, Hamel-Bravo, Magdalena J., Bayliss, Matthew B., Gladders, Michael D., López, Sebastián, Tejos, Nicolás
The hydrogen Lyman-alpha (Lya) emission line, the brightest spectral feature of a photoionized gas, is considered an indirect tracer of the escape of Lyman continuum (LyC) photons, particularly when the intergalactic medium is too opaque for direct d
Externí odkaz:
http://arxiv.org/abs/2409.10604
Autor:
Monter, Silvia Almada, Gronke, Max
The diverse Lyman-alpha (Ly$\alpha$) line profiles are essential probes of gas in and around galaxies. While isotropic models can successfully reproduce a range of Ly$\alpha$ observables, the correspondence between the model and actual physical param
Externí odkaz:
http://arxiv.org/abs/2404.07169
Autor:
Chang, Seok-Jun, Gronke, Max
The Mg II resonance doublet at 2796 {\AA} and 2803 {\AA} is an increasingly important tool to study cold, $T \sim 10^{4}\,$K, gas -- an observational driven development requiring theoretical support. We develop a new Monte Carlo radiative transfer co
Externí odkaz:
http://arxiv.org/abs/2403.11524
Lyman-$\alpha$ (Ly$\alpha$) is the strongest emission line in the accretion-generated UV spectra from T-Tauri stars and, as such, plays a critical role in regulating chemistry within the surrounding protoplanetary disks. Due to its resonant nature, t
Externí odkaz:
http://arxiv.org/abs/2310.14477
Autor:
Forero-Romero, Jaime E., Gronke, Max, Remolina-Gutiérrez, Maria Camila, Garavito-Camargo, Nicolás, Dijkstra, Mark
Star-forming compact dwarf galaxies (CDGs) resemble the expected pristine conditions of the first galaxies in the Universe and are the best systems to test models on primordial galaxy formation and evolution. Here, we report on one of such CDGs, Tolo
Externí odkaz:
http://hdl.handle.net/10150/627137
http://arizona.openrepository.com/arizona/handle/10150/627137
http://arizona.openrepository.com/arizona/handle/10150/627137
Autor:
Lobos, Vale González, Battaia, Fabrizio Arrigoni, Chang, Seok-Jun, Gronke, Max, Kauffmann, Guinevere, Chen, Chian-Chou, Fu, Hai, Obreja, Aura, Farina, Emanuele P.
Publikováno v:
A&A 679, A41 (2023)
We present VLT/MUSE observations targeting the extended Lyman-$\alpha$ (Ly$\alpha$) emission of five high-redshift ($z\sim$3-4) submillimeter galaxies (SMGs) with increasing quasar (QSO) radiation: two SMGs, two SMGs hosting a QSO, and one SMG hostin
Externí odkaz:
http://arxiv.org/abs/2308.15955
Autor:
Das, Hitesh Kishore, Gronke, Max
Both multiphase gas and magnetic fields are ubiquitous in astrophysics. However, the influence of magnetic fields on mixing of the different phases is still largely unexplored. In this study, we use both turbulent radiative mixing layer (TRML) and tu
Externí odkaz:
http://arxiv.org/abs/2307.06411
Autor:
Hu, Weida, Martin, Crystal L., Gronke, Max, Gazagnes, Simon, Hayes, Matthew, Chisholm, John, Heckman, Timothy, Mingozzi, Matilde, Roy, Namrata, Senchyna, Peter, Xu, Xinfeng, Berg, Danielle A., James, Bethan L., Stark, Daniel P., Arellano-Córdova, Karla Z., Henry, Alaina, Jaskot, Anne E., Kumari, Nimisha, Parker, Kaelee S., Scarlata, Claudia, Wofford, Aida, Amorín, Ricardo O., Leonhardes-Barboza, Naunet, Brinchmann, Jarle, Carr, Cody
Lyman-alpha line profiles are a powerful probe of ISM structure, outflow speed, and Lyman continuum escape fraction. In this paper, we present the Ly$\alpha$ line profiles of the COS Legacy Archive Spectroscopic SurveY, a sample rich in spectroscopic
Externí odkaz:
http://arxiv.org/abs/2307.04911
We present a new semi-analytic formalism for modeling metal absorption lines that emerge from a clumpy galactic environment, ALPACA. We predict the ''down-the-barrel'' (DTB) metal absorption line profiles and the EW of absorption at different impact
Externí odkaz:
http://arxiv.org/abs/2306.11089