Zobrazeno 1 - 10
of 191
pro vyhledávání: '"B. Fielding"'
Publikováno v:
The Astrophysical Journal, Vol 972, Iss 2, p 148 (2024)
We present CloudFlex , an open-source tool for predicting absorption-line signatures of cool gas in galaxy halos with small-scale structure. Motivated by analyses of ∼10 ^4 K material in hydrodynamical simulations of turbulent, multiphase media, we
Externí odkaz:
https://doaj.org/article/1a34eca9adda439db229e813246394f5
Autor:
Chang-Goo Kim, Eve C. Ostriker, Jeong-Gyu Kim, Munan Gong, Greg L. Bryan, Drummond B. Fielding, Sultan Hassan, Matthew Ho, Sarah M. R. Jeffreson, Rachel S. Somerville, Ulrich P. Steinwandel
Publikováno v:
The Astrophysical Journal, Vol 972, Iss 1, p 67 (2024)
We present a new suite of numerical simulations of the star-forming interstellar medium (ISM) in galactic disks using the TIGRESS-NCR framework. Distinctive aspects of our simulation suite are (1) sophisticated and comprehensive numerical treatments
Externí odkaz:
https://doaj.org/article/7d79445bc0264c139ce37b8908883784
Publikováno v:
The Astrophysical Journal, Vol 966, Iss 2, p 181 (2024)
Turbulent radiative mixing layers play an important role in many astrophysical contexts where cool (≲10 ^4 K) clouds interact with hot flows (e.g., galactic winds, high-velocity clouds, infalling satellites in halos and clusters). The fate of these
Externí odkaz:
https://doaj.org/article/db547a11cced4fda85b11a994a3b488d
Autor:
Ulrich P. Steinwandel, Chang-Goo Kim, Greg L. Bryan, Eve C. Ostriker, Rachel S. Somerville, Drummond B. Fielding
Publikováno v:
The Astrophysical Journal, Vol 960, Iss 2, p 100 (2024)
We present the first results from a high-resolution simulation with a focus on galactic wind driving for an isolated galaxy with a halo mass of ∼10 ^11 M _⊙ (similar to the Large Magellanic Cloud) and a total gas mass of ∼6 × 10 ^8 M _⊙ , re
Externí odkaz:
https://doaj.org/article/c23d5a25575c48fdb6c7ae4843494207
Autor:
Dorota Sabat‐Pośpiech, Kim Fabian‐Kolpanowicz, Helen Kalirai, Natalie Kipling, Sarah E Coupland, Judy M Coulson, Andrew B Fielding
Publikováno v:
The Journal of Pathology: Clinical Research, Vol 8, Iss 4, Pp 383-394 (2022)
Abstract Uveal melanoma (UM) is the most common intraocular cancer in adults. Whilst treatment of primary UM (PUM) is often successful, around 50% of patients develop metastatic disease with poor outcomes, linked to chromosome 3 loss (monosomy 3, M3)
Externí odkaz:
https://doaj.org/article/e52134711fec4d00857b44a97422ee2d
Publikováno v:
The Astrophysical Journal Letters, Vol 949, Iss 1, p L5 (2023)
The processes controlling the complex clump structure, phase distribution, and magnetic field geometry that develop across a broad range of scales in the turbulent interstellar medium (ISM) remain unclear. Using unprecedentedly high-resolution 3D mag
Externí odkaz:
https://doaj.org/article/768586b1cbb14e7588759791ed143a43
Autor:
Viraj Pandya, Drummond B. Fielding, Greg L. Bryan, Christopher Carr, Rachel S. Somerville, Jonathan Stern, Claude-André Faucher-Giguère, Zachary Hafen, Daniel Anglés-Alcázar, John C. Forbes
Publikováno v:
The Astrophysical Journal, Vol 956, Iss 2, p 118 (2023)
The circumgalactic medium (CGM) plays a pivotal role in regulating gas flows around galaxies and thus shapes their evolution. However, the details of how galaxies and their CGM coevolve remain poorly understood. We present a new time-dependent two-zo
Externí odkaz:
https://doaj.org/article/7dc2c8b8049c45e1bfa58c84ea84be67
Publikováno v:
The Astrophysical Journal, Vol 950, Iss 2, p 91 (2023)
Turbulent radiative mixing layers (TRMLs) form at the interface of cold, dense gas and hot, diffuse gas in motion with each other. TRMLs are ubiquitous in and around galaxies on a variety of scales, including galactic winds and the circumgalactic med
Externí odkaz:
https://doaj.org/article/9f7cb3c1badd4e198c0e4174c56ba836
Publikováno v:
The Astrophysical Journal, Vol 949, Iss 1, p 21 (2023)
Galactic outflows driven by supernovae (SNe) are thought to be a powerful regulator of a galaxy’s star-forming efficiency. Mass, energy, and metal outflows ( η _M , η _E , and η _Z , here normalized by the star formation rate, the SNe energy, an
Externí odkaz:
https://doaj.org/article/7e667a3ab5134daba1bf4cd450864a61