Circumgalactic Medium on the Largest Scales: Detecting X-Ray
Absorption Lines with Large-area Microcalorimeters

J 2023

Circumgalactic Medium on the Largest Scales: Detecting X-Ray Absorption Lines with Large-area Microcalorimeters

BOGDAN, Akos, Ildar KHABIBULLIN, Orsolya Eszter KOVÁCS, Gerrit SCHELLENBERGER, John ZUHONE et. al.

Základní údaje

Originální název

Circumgalactic Medium on the Largest Scales: Detecting X-Ray Absorption Lines with Large-area Microcalorimeters

Autoři

BOGDAN, Akos, Ildar KHABIBULLIN, Orsolya Eszter KOVÁCS (348 Maďarsko, domácí), Gerrit SCHELLENBERGER, John ZUHONE, Joseph N. BURCHETT, Klaus DOLAG, Eugene CHURAZOV, William R. FORMAN, Christine JONES, Caroline KILBOURNE, Ralph P. KRAFT, Erwin LAU, Maxim MARKEVITCH, Dan MCCAMMON, Daisuke NAGAI, Dylan NELSON, Anna OGORZALEK, Benjamin D. OPPENHEIMER, Arnab SARKAR, Yuanyuan SU, Nhut TRUONG, Sylvain VEILLEUX, Stephan VLADUTESCU-ZOPP a Irina ZHURAVLEVA

Vydání

Astrophysical Journal, IOP Publishing Ltd, 2023, 0004-637X

Další údaje

Jazyk

angličtina

Typ výsledku

Článek v odborném periodiku

Obor

10308 Astronomy

Stát vydavatele

Velká Británie a Severní Irsko

Utajení

není předmětem státního či obchodního tajemství

Odkazy

URL arXiv

Impakt faktor

Impact factor: 4.900 v roce 2022

Kód RIV

RIV/00216224:14310/23:00134378

Organizační jednotka

Přírodovědecká fakulta

DOI

http://dx.doi.org/10.3847/1538-4357/acdeec

UT WoS

001041282500001

Klíčová slova anglicky

Circumgalactic medium; Disk galaxies; Galaxy evolution; High resolution spectroscopy; X-ray astronomy; X-ray observatories; X-ray sources

Štítky

rivok

Příznaky

Mezinárodní význam, Recenzováno

Změněno: 16. 1. 2024 09:09, Mgr. Marie Šípková, DiS.

Anotace

V originále

The circumgalactic medium (CGM) plays a crucial role in galaxy evolution as it fuels star formation, retains metals ejected from the galaxies, and hosts gas flows in and out of galaxies. For Milky Way–type and more-massive galaxies, the bulk of the CGM is in hot phases best accessible at X-ray wavelengths. However, our understanding of the CGM remains largely unconstrained due to its tenuous nature. A promising way to probe the CGM is via X-ray absorption studies. Traditional absorption studies utilize bright background quasars, but this method probes the CGM in a pencil beam, and, due to the rarity of bright quasars, the galaxy population available for study is limited. Large-area, high spectral resolution X-ray microcalorimeters offer a new approach to exploring the CGM in emission and absorption. Here, we demonstrate that the cumulative X-ray emission from cosmic X-ray background sources can probe the CGM in absorption. We construct column density maps of major X-ray ions from the Magneticum simulation and build realistic mock images of nine galaxies to explore the detectability of X-ray absorption lines arising from the large-scale CGM. We conclude that the O VII absorption line is detectable around individual massive galaxies at the 3σ–6σ confidence level. For Milky Way–type galaxies, the O VII and O VIII absorption lines are detectable at the ∼ 6σ and ∼ 3σ levels even beyond the virial radius when coadding data from multiple galaxies. This approach complements emission studies, does not require additional exposures, and will allow for probing the baryon budget and the CGM at the largest scales.

Návaznosti

GX21-13491X, projekt VaV

Název: Zkoumání žhavého vesmíru a porozumění kosmické zpětné vazbě (Akronym: EHU)

Investor: Grantová agentura ČR, Exploring the Hot Universe and Understanding Comic Feedback

Citovat

BOGDAN, Akos, Ildar KHABIBULLIN, Orsolya Eszter KOVÁCS, Gerrit SCHELLENBERGER, John ZUHONE, Joseph N. BURCHETT, Klaus DOLAG, Eugene CHURAZOV, William R. FORMAN, Christine JONES, Caroline KILBOURNE, Ralph P. KRAFT, Erwin LAU, Maxim MARKEVITCH, Dan MCCAMMON, Daisuke NAGAI, Dylan NELSON, Anna OGORZALEK, Benjamin D. OPPENHEIMER, Arnab SARKAR, Yuanyuan SU, Nhut TRUONG, Sylvain VEILLEUX, Stephan VLADUTESCU-ZOPP a Irina ZHURAVLEVA. Circumgalactic Medium on the Largest Scales: Detecting X-Ray Absorption Lines with Large-area Microcalorimeters. Astrophysical Journal. IOP Publishing Ltd, 2023, roč. 953, č. 1, s. 1-16. ISSN 0004-637X. Dostupné z: https://dx.doi.org/10.3847/1538-4357/acdeec.

@article{2361462,
   author = {Bogdan, Akos and Khabibullin, Ildar and Kovács, Orsolya Eszter and Schellenberger, Gerrit and ZuHone, John and Burchett, Joseph N. and Dolag, Klaus and Churazov, Eugene and Forman, William R. and Jones, Christine and Kilbourne, Caroline and Kraft, Ralph P. and Lau, Erwin and Markevitch, Maxim and McCammon, Dan and Nagai, Daisuke and Nelson, Dylan and Ogorzalek, Anna and Oppenheimer, Benjamin D. and Sarkar, Arnab and Su, Yuanyuan and Truong, Nhut and Veilleux, Sylvain and VladutescuandZopp, Stephan and Zhuravleva, Irina},
   article_number = {1},
   doi = {http://dx.doi.org/10.3847/1538-4357/acdeec},
   keywords = {Circumgalactic medium; Disk galaxies; Galaxy evolution; High resolution spectroscopy; X-ray astronomy; X-ray observatories; X-ray sources},
   language = {eng},
   issn = {0004-637X},
   journal = {Astrophysical Journal},
   title = {Circumgalactic Medium on the Largest Scales: Detecting X-Ray Absorption Lines with Large-area Microcalorimeters},
   url = {https://doi.org/10.3847/1538-4357/acdeec},
   volume = {953},
   year = {2023}
}

TY  - JOUR
ID  - 2361462
AU  - Bogdan, Akos - Khabibullin, Ildar - Kovács, Orsolya Eszter - Schellenberger, Gerrit - ZuHone, John - Burchett, Joseph N. - Dolag, Klaus - Churazov, Eugene - Forman, William R. - Jones, Christine - Kilbourne, Caroline - Kraft, Ralph P. - Lau, Erwin - Markevitch, Maxim - McCammon, Dan - Nagai, Daisuke - Nelson, Dylan - Ogorzalek, Anna - Oppenheimer, Benjamin D. - Sarkar, Arnab - Su, Yuanyuan - Truong, Nhut - Veilleux, Sylvain - Vladutescu-Zopp, Stephan - Zhuravleva, Irina
PY  - 2023
TI  - Circumgalactic Medium on the Largest Scales: Detecting X-Ray Absorption Lines with Large-area Microcalorimeters
JF  - Astrophysical Journal
VL  - 953
IS  - 1
SP  - 1-16
EP  - 1-16
PB  - IOP Publishing Ltd
SN  - 0004637X
KW  - Circumgalactic medium
KW  - Disk galaxies
KW  - Galaxy evolution
KW  - High resolution spectroscopy
KW  - X-ray astronomy
KW  - X-ray observatories
KW  - X-ray sources
UR  - https://doi.org/10.3847/1538-4357/acdeec
N2  - The circumgalactic medium (CGM) plays a crucial role in galaxy evolution as it fuels star formation, retains metals ejected from the galaxies, and hosts gas flows in and out of galaxies. For Milky Way–type and more-massive galaxies, the bulk of the CGM is in hot phases best accessible at X-ray wavelengths. However, our understanding of the CGM remains largely unconstrained due to its tenuous nature. A promising way to probe the CGM is via X-ray absorption studies. Traditional absorption studies utilize bright background quasars, but this method probes the CGM in a pencil beam, and, due to the rarity of bright quasars, the galaxy population available for study is limited. Large-area, high spectral resolution X-ray microcalorimeters offer a new approach to exploring the CGM in emission and absorption. Here, we demonstrate that the cumulative X-ray emission from cosmic X-ray background sources can probe the CGM in absorption. We construct column density maps of major X-ray ions from the Magneticum simulation and build realistic mock images of nine galaxies to explore the detectability of X-ray absorption lines arising from the large-scale CGM. We conclude that the O VII absorption line is detectable around individual massive galaxies at the 3σ–6σ confidence level. For Milky Way–type galaxies, the O VII and O VIII absorption lines are detectable at the ∼ 6σ and ∼ 3σ levels even beyond the virial radius when coadding data from multiple galaxies. This approach complements emission studies, does not require additional exposures, and will allow for probing the baryon budget and the CGM at the largest scales.
ER  -

BOGDAN, Akos, Ildar KHABIBULLIN, Orsolya Eszter KOVÁCS, Gerrit SCHELLENBERGER, John ZUHONE, Joseph N. BURCHETT, Klaus DOLAG, Eugene CHURAZOV, William R. FORMAN, Christine JONES, Caroline KILBOURNE, Ralph P. KRAFT, Erwin LAU, Maxim MARKEVITCH, Dan MCCAMMON, Daisuke NAGAI, Dylan NELSON, Anna OGORZALEK, Benjamin D. OPPENHEIMER, Arnab SARKAR, Yuanyuan SU, Nhut TRUONG, Sylvain VEILLEUX, Stephan VLADUTESCU-ZOPP a Irina ZHURAVLEVA. Circumgalactic Medium on the Largest Scales: Detecting X-Ray Absorption Lines with Large-area Microcalorimeters. \textit{Astrophysical Journal}. IOP Publishing Ltd, 2023, roč.~953, č.~1, s.~1-16. ISSN~0004-637X. Dostupné z: https://dx.doi.org/10.3847/1538-4357/acdeec.

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