Correlations between supermassive black holes and hot gas atmospheres in IllustrisTNG and X-ray observations

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F21%3A00118860" target="_blank" >RIV/00216224:14310/21:00118860 - isvavai.cz</a>

Výsledek na webu

<a href="https://doi.org/10.1093/mnras/staa3880" target="_blank" >https://doi.org/10.1093/mnras/staa3880</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1093/mnras/staa3880" target="_blank" >10.1093/mnras/staa3880</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Correlations between supermassive black holes and hot gas atmospheres in IllustrisTNG and X-ray observations

Popis výsledku v původním jazyce

Recent X-ray observations have revealed remarkable correlations between the masses of central supermassive black holes (SMBHs) and the X-ray properties of the hot atmospheres permeating their host galaxies, thereby indicating the crucial role of the atmospheric gas in tracing SMBH growth in the high-mass regime. We examine this topic theoretically using the IllustrisTNG cosmological simulations and provide insights to the nature of this SMBH - gaseous halo connection. By carrying out a mock X-ray analysis for a mass-selected sample of TNG100 simulated galaxies at z = 0, we inspect the relationship between the masses of SMBHs and the hot gas temperatures and luminosities at various spatial and halo scales - from galactic (similar to R-e) to group/cluster scales (similar to R-500c). We find strong SMBH-X-ray correlations mostly in quenched galaxies and find that the correlations become stronger and tighter at larger radii. Critically, the X-ray temperature (k(B)T(X)) at large radii (r greater than or similar to 5R(e)) traces the SMBH mass with a remarkably small scatter (similar to 0.2 dex). The relations emerging from IllustrisTNG are broadly consistent with those obtained from recent X-ray observations. Overall, our analysis suggests that, within the framework of IllustrisTNG, the present-time M-BH-k(B)T(X) correlations at the high-mass end (M-BH greater than or similar to 10(8)M(circle dot)) are fundamentally a reflection of the SMBH mass-halo mass relation, which at such high masses is set by the hierarchical assembly of structures. The exact form, locus, and scatter of those scaling relations are, however, sensitive to feedback processes such as those driven by star formation and SMBH activity.

Název v anglickém jazyce

Correlations between supermassive black holes and hot gas atmospheres in IllustrisTNG and X-ray observations

Popis výsledku anglicky

Recent X-ray observations have revealed remarkable correlations between the masses of central supermassive black holes (SMBHs) and the X-ray properties of the hot atmospheres permeating their host galaxies, thereby indicating the crucial role of the atmospheric gas in tracing SMBH growth in the high-mass regime. We examine this topic theoretically using the IllustrisTNG cosmological simulations and provide insights to the nature of this SMBH - gaseous halo connection. By carrying out a mock X-ray analysis for a mass-selected sample of TNG100 simulated galaxies at z = 0, we inspect the relationship between the masses of SMBHs and the hot gas temperatures and luminosities at various spatial and halo scales - from galactic (similar to R-e) to group/cluster scales (similar to R-500c). We find strong SMBH-X-ray correlations mostly in quenched galaxies and find that the correlations become stronger and tighter at larger radii. Critically, the X-ray temperature (k(B)T(X)) at large radii (r greater than or similar to 5R(e)) traces the SMBH mass with a remarkably small scatter (similar to 0.2 dex). The relations emerging from IllustrisTNG are broadly consistent with those obtained from recent X-ray observations. Overall, our analysis suggests that, within the framework of IllustrisTNG, the present-time M-BH-k(B)T(X) correlations at the high-mass end (M-BH greater than or similar to 10(8)M(circle dot)) are fundamentally a reflection of the SMBH mass-halo mass relation, which at such high masses is set by the hierarchical assembly of structures. The exact form, locus, and scatter of those scaling relations are, however, sensitive to feedback processes such as those driven by star formation and SMBH activity.

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10308 - Astronomy (including astrophysics,space science)

Projekt

<a href="/cs/project/GX21-13491X" target="_blank" >GX21-13491X: Zkoumání žhavého vesmíru a porozumění kosmické zpětné vazbě</a><br>

Návaznosti

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>S - Specificky vyzkum na vysokych skolach

Rok uplatnění

2021

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název periodika

Monthly Notices of the Royal Astronomical Society

ISSN

0035-8711

e-ISSN

1365-2966

Svazek periodika

501

Číslo periodika v rámci svazku

2

Stát vydavatele periodika

GB - Spojené království Velké Británie a Severního Irska

Počet stran výsledku

21

Strana od-do

2210-2230

Kód UT WoS článku

000608475600045

EID výsledku v databázi Scopus

2-s2.0-85100264120