All

What are you looking for?

All
Projects
Results
Organizations

Quick search

  • Projects supported by TA ČR
  • Excellent projects
  • Projects with the highest public support
  • Current projects

Smart search

  • That is how I find a specific +word
  • That is how I leave the -word out of the results
  • “That is how I can find the whole phrase”

The relation between accretion rate and jet power in early-type galaxies with thermally unstable hot atmospheres

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F22%3A00564026" target="_blank" >RIV/67985815:_____/22:00564026 - isvavai.cz</a>

  • Alternative codes found

    RIV/00216224:14310/22:00127110

  • Result on the web

    <a href="https://doi.org/10.1093/mnras/stac2770" target="_blank" >https://doi.org/10.1093/mnras/stac2770</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1093/mnras/stac2770" target="_blank" >10.1093/mnras/stac2770</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    The relation between accretion rate and jet power in early-type galaxies with thermally unstable hot atmospheres

  • Original language description

    We use Chandra X-ray data and Very Large Array radio observations for a sample of 20 nearby, massive, X-ray bright, early-type galaxies to investigate the relation between the Bondi accretion rates and the mechanical jet powers. We find a strong correlation (rho = 0.96(-0.09)(+0.03), BF10 > 100) between the Bondi accretion power, P-Bondi, and the mechanical jet power, P-jet, for a subsample of 14 galaxies, which also host cool H alpha+[N II] line emitting gas and thus likely have thermally unstable atmospheres. The relation between the Bondi accretion power and the mechanical jet power for this subsample is well described by a power-law model log P-Bondi/10(43) erg s(-1) = alpha + beta log P-jet/10(43) erg s(-1), where alpha = 1.10 +/- 0.25 and beta = 1.10 +/- 0.24 with an intrinsic scatter sigma = 0.08(-0.06)(+0.14) dex. The results indicate that in all galaxies with thermally unstable atmospheres the cooling atmospheric gas feeds the central black holes at a similar jet-to-Bondi power ratio. For the full sample of 20 galaxies, the correlation is weaker and in a subset of galaxies with no signs of H alpha+[N II] emission, we see a hint for a systematically lower jet-to-Bondi power ratio. We also investigate the dependence of jet power on individual quantities in the Bondi formula such as the supermassive black hole mass (M-center dot) and the specific entropy of the gas (K) at the Bondi radius. For the subsample of H alpha+[N II] emitting galaxies, we find a very tight correlation of P-jet with M-center dot (rho = 0.91(-0.11)(+0.06), BF10 > 100) and, although poorly constrained, a hint of an anticorrelation for P-jet and K (rho =0.47(-0.37)(+0.60), BF10 = 1.1).

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    <a href="/en/project/GX21-13491X" target="_blank" >GX21-13491X: Exploring the Hot Universe and Understanding Cosmic Feedback</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2022

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Monthly Notices of the Royal Astronomical Society

  • ISSN

    0035-8711

  • e-ISSN

    1365-2966

  • Volume of the periodical

    517

  • Issue of the periodical within the volume

    3

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    29

  • Pages from-to

    3682-3710

  • UT code for WoS article

    000874073200003

  • EID of the result in the Scopus database

    2-s2.0-85145260008