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Properties of the Hot Ambient Medium of Early-type Galaxies Hosting Powerful Radio Sources

Identifikátory výsledku

  • Kód výsledku v IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F20%3A00116462" target="_blank" >RIV/00216224:14310/20:00116462 - isvavai.cz</a>

  • Výsledek na webu

    <a href="https://iopscience.iop.org/article/10.3847/1538-4357/aba8a8/pdf" target="_blank" >https://iopscience.iop.org/article/10.3847/1538-4357/aba8a8/pdf</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.3847/1538-4357/aba8a8" target="_blank" >10.3847/1538-4357/aba8a8</a>

Alternativní jazyky

  • Jazyk výsledku

    angličtina

  • Název v původním jazyce

    Properties of the Hot Ambient Medium of Early-type Galaxies Hosting Powerful Radio Sources

  • Popis výsledku v původním jazyce

    We present an archival analysis of Chandra X-ray observations for 12 nearby early-type galaxies hosting radio sources with radio power &gt;10(23)W Hz(-1)at 1.4 GHz, similar to the radio power of the radio source in NGC 4261. Previously, in a similar analysis of eight nearby X-ray and optically bright elliptical galaxies, Werner et al. found that NGC 4261 exhibited unusually low central gas entropy compared to the full sample. In the central 0.3 kpc of NGC 4261, the ratio of cooling time to freefall time (t(cool)/t(ff)) is less than 10, indicating that cold clouds may be precipitating out of the hot ambient medium and providing fuel for accretion in the central region. NGC 4261 also hosts the most powerful radio source in the original sample. Because NGC 4261 may represent an important phase during which powerful feedback from a central active galactic nucleus (AGN) is fueled by multiphase condensation in the central kiloparsec, we searched the Chandra archive for analogs to NGC 4261. We present entropy profiles of those galaxies, as well as profiles oft(cool)/t(ff). We find that one of them, IC 4296, exhibits properties similar to NGC 4261, including the presence of only single-phase gas outside ofr similar to 2 kpc and a similar central velocity dispersion. We compare the properties of NGC 4261 and IC 4296 to hydrodynamic simulations of AGN feedback fueled by precipitation. Over the course of those simulations, the single-phase galaxy has an entropy gradient that remains similar to the entropy profiles inferred from our observations.

  • Název v anglickém jazyce

    Properties of the Hot Ambient Medium of Early-type Galaxies Hosting Powerful Radio Sources

  • Popis výsledku anglicky

    We present an archival analysis of Chandra X-ray observations for 12 nearby early-type galaxies hosting radio sources with radio power &gt;10(23)W Hz(-1)at 1.4 GHz, similar to the radio power of the radio source in NGC 4261. Previously, in a similar analysis of eight nearby X-ray and optically bright elliptical galaxies, Werner et al. found that NGC 4261 exhibited unusually low central gas entropy compared to the full sample. In the central 0.3 kpc of NGC 4261, the ratio of cooling time to freefall time (t(cool)/t(ff)) is less than 10, indicating that cold clouds may be precipitating out of the hot ambient medium and providing fuel for accretion in the central region. NGC 4261 also hosts the most powerful radio source in the original sample. Because NGC 4261 may represent an important phase during which powerful feedback from a central active galactic nucleus (AGN) is fueled by multiphase condensation in the central kiloparsec, we searched the Chandra archive for analogs to NGC 4261. We present entropy profiles of those galaxies, as well as profiles oft(cool)/t(ff). We find that one of them, IC 4296, exhibits properties similar to NGC 4261, including the presence of only single-phase gas outside ofr similar to 2 kpc and a similar central velocity dispersion. We compare the properties of NGC 4261 and IC 4296 to hydrodynamic simulations of AGN feedback fueled by precipitation. Over the course of those simulations, the single-phase galaxy has an entropy gradient that remains similar to the entropy profiles inferred from our observations.

Klasifikace

  • Druh

    J<sub>imp</sub> - Článek v periodiku v databázi Web of Science

  • CEP obor

  • OECD FORD obor

    10308 - Astronomy (including astrophysics,space science)

Návaznosti výsledku

  • Projekt

  • Návaznosti

    S - Specificky vyzkum na vysokych skolach

Ostatní

  • Rok uplatnění

    2020

  • Kód důvěrnosti údajů

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

Údaje specifické pro druh výsledku

  • Název periodika

    Astrophysical Journal

  • ISSN

    0004-637X

  • e-ISSN

  • Svazek periodika

    899

  • Číslo periodika v rámci svazku

    2

  • Stát vydavatele periodika

    US - Spojené státy americké

  • Počet stran výsledku

    10

  • Strana od-do

    1-10

  • Kód UT WoS článku

    000565748200001

  • EID výsledku v databázi Scopus

    2-s2.0-85090421256