Article
Astronomy & Astrophysics
Alexander Beckettt, Simon L. Morris, Michele Fumagalli, Nicolas Tejos, Buell Jannuzi, Sebastiano Cantalupo
Summary: We use H i absorption to model potential disc and outflow structures in the circumgalactic medium, and find possible outflows and co-rotating structures, suggesting that geometric cuts are not sufficient to distinguish between discs and outflows in single line-of-sight studies.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Martin Wendt, Nicolas F. Bouche, Johannes Zabl, Ilane Schroetter, Sowgat Muzahid
Summary: The study investigates the dust content of the circum-galactic medium (CGM) in relation to the position of quasar sightlines with respect to the galaxy major-axis. It finds a positive correlation between the azimuthal angle and [Zn/Fe], indicating that CGM along the minor axis is on average more metal enriched compared to the gas located along the major axis. This anisotropic distribution is consistent with recent results on outflow and accretion in hydro-dynamical simulations.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Sowgat Muzahid, Joop Schaye, Sebastiano Cantalupo, Raffaella Anna Marino, Nicolas F. Bouche, Sean Johnson, Michael Maseda, Martin Wendt, Lutz Wisotzki, Johannes Zabl
Summary: The first characterization of the circumgalactic medium of Ly alpha emitters (LAEs) reveals distinct features in terms of luminosity and interstellar material absorption, with no strong dependence of absorption on transverse distance, redshift, or Ly alpha emission line properties. However, a correlation is found between increased absorption near LAEs with higher star formation rates, suggesting a link between surrounding interstellar hydrogen and star formation in LAEs.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Pratyush Anshul, Anand Narayanan, Sowgat Muzahid, Alexander Beckett, Simon L. Morris
Summary: This study presents the physical properties, chemical abundances, and transverse sizes of a multiphase medium in a galaxy field at z = 0.399 using HST/COS spectra of the twin quasar lines of sight Q 0107-025A & Q 0107-025B. The absorber towards Q 0107-025B is a partial Lyman limit system (pLLS) while the absorber along the other sightline has a lower HI column density. OVI and broad HI coinciding in both sightlines are best explained through collisional ionization in a cooling plasma with solar metallicity.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Huanqing Chen, Rupert A. C. Croft, Nickolay Y. Gnedin
Summary: In this study, a convolutional neural network (CNN) method is used to recover the temperature distribution around quasars and estimate their lifetimes. The results show that the simple CNN can accurately recover the temperature profile with an accuracy of approximately 1400K in an idealized case. However, observational noise poses a significant challenge and can reduce the accuracy to approximately 2340K even with high signal-to-noise spectra.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
A. D. Amaral, T. Vernstrom, B. M. Gaensler
Summary: Researchers conducted an analysis on the statistical characteristics of weak magnetic fields in the intergalactic medium, but did not detect a significant correlation signal. They determined model-dependent upper limits on the parallel magnetic field strength of filaments in the IGM, and noted that these results are consistent with previous findings.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Thomas J. Cooper, Gwen C. Rudie, Hsiao-Wen Chen, Sean D. Johnson, Fakhri S. Zahedy, Mandy C. Chen, Erin Boettcher, Gregory L. Walth, Sebastiano Cantalupo, Kathy L. Cooksey, Claude-Andre Faucher-Giguere, Jenny E. Greene, Sebastian Lopez, John S. Mulchaey, Steven Penton, Patrick Petitjean, Mary E. Putman, Marc Rafelski, Michael Rauch, Joop Schaye, Robert A. Simcoe
Summary: This study investigates two partial Lyman limit systems (pLLSs) discovered in the Cosmic Ultraviolet Baryon Survey (CUBS), providing detailed information on the ionization analysis of multiphase gas in diverse galaxy environments. The data reveal kinematically aligned gas components with varying chemical abundances and densities, stressing the importance of considering the heterogeneous nature of circumgalactic gas in theoretical models. Additionally, survey data point to these systems being located near star-forming galaxies, highlighting the significance of studying the gas surrounding galaxies.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Zhijie Qu, Hsiao-Wen Chen, Gwen C. Rudie, Fakhri S. Zahedy, Sean D. Johnson, Erin Boettcher, Sebastiano Cantalupo, Mandy C. Chen, Kathy L. Cooksey, David DePalma, Claude-Andre Faucher-Giguere, Michael Rauch, Joop Schaye, Robert A. Simcoe
Summary: This paper presents a systematic study of the photoionization and thermodynamic properties of the cool circumgalactic medium (CGM) around galaxies at redshift z less than or similar to 1, providing important insights into the gas density, temperature, and pressure of individual absorbing components and their non-thermal motions.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Margherita Molaro, Vid Irsic, James S. Bolton, Maggie Lieu, Laura C. Keating, Ewald Puchwein, Martin G. Haehnelt, Matteo Viel
Summary: Inhomogeneous reionization increases the power spectrum of the 1D Ly alpha forest at large scales at redshifts z >= 4. This is due to coherent fluctuations in the ionized hydrogen fraction resulting from large-scale variations in post-reionization gas temperature. An analysis of Ly alpha forest power spectrum measurements at 4.0 <= z <= 4.6 suggests a preference for a large-scale enhancement, potentially indicating inhomogeneous reionization. Future power spectrum measurements with lower uncertainties should provide more conclusive evidence for this enhancement.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Sean Morrison, Matthew M. Pieri, Debopam Som, Ignasi Perez-Rafols
Summary: The study investigates large-scale UV background inhomogeneities associated with high redshift quasar populations by measuring metal absorption in quasar absorption spectrum stacking. Stronger high ionization species absorption is observed closer to quasars at 2.4 < z < 3.1. Additionally, weak signs of increasing homogeneity with time are explored in the range of 2.05 < z < 2.4. Limitations of incomplete quasar samples are noted in the interpretation of results.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Lydia Stofanova, Aurora Simionescu, Nastasha A. Wijers, Joop Schaye, Jelle S. Kaastra
Summary: This paper studies the ionization effects of radiation from galaxy clusters and the cosmic background on a very tenuous plasma, and the challenge of modeling the spectral features due to photoionization. The ionization fractions obtained by considering the cosmic background as well as the distance from the emission source are discussed. The changes in column densities for different lines of sight passing close to the cluster outskirts are also predicted.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
David Spence, Massimiliano Bonamente, Jukka Nevalainen, Toni Tuominen, Jussi Ahoranta, Jelle de Plaa, Wenhao Liu, Nastasha Wijers
Summary: This paper analyzes the X-ray spectra of the quasar 1ES 1553+113 in search of absorption lines from the WHIM. The study detects a possible O vii absorption line at redshift z ~ 0.1877 with a 2.6 sigma confidence level. However, further analysis does not find evidence for additional X-ray absorbing WHIM. The paper also presents a statistical framework for cosmological inferences from absorption line analysis.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Hiroyuki Hirashita, Ting-Wen Lan
Summary: Observations of reddening in the circum-galactic medium suggest a significant presence of small grains, possibly produced through the shattering of pre-existing large grains. Physical conditions in cool clumps are favorable for small-grain production, explaining the observed reddening phenomenon.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Prakash Gaikwad, Martin G. Haehnelt, Fredrick B. Davies, Sarah E. Bosman, Margherita Molaro, Girish Kulkarni, Valentina D'Odorico, George D. Becker, Rebecca L. Davies, Fahad Nasir, James S. Bolton, Laura C. Keating, Vid Irsic, Ewald Puchwein, Yongda Zhu, Shikhar Asthana, Jinyi Yang, Samuel Lai, Anna-Christina Eilers
Summary: In this study, we measured the mean free path, photoionization rate, and neutral fraction of hydrogen at different redshifts using QSO absorption spectra. We compared our results with simulations and found significant evolution of these parameters with increasing redshift.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Rebecca L. Davies, E. Ryan-Weber, V D'Odorico, S. E. Bosman, R. A. Meyer, G. D. Becker, G. Cupani, M. Bischetti, A. M. Sebastian, A-C Eilers, E. P. Farina, F. Wang, J. Yang, Y. Zhu
Summary: This article investigates the ionization state and chemical composition of circumgalactic and intergalactic gas near the end of the reionization epoch by studying metal absorption lines in the spectra of distant quasars. With a sample of 30 luminous quasars, the authors construct a catalogue of 778 systems showing absorption in various elements, which significantly expands on existing samples and provides important insights into the early Universe.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)