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Powerful AGN jets and unbalanced cooling in the hot atmosphere of IC 4296

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F19%3A00110293" target="_blank" >RIV/00216224:14310/19:00110293 - isvavai.cz</a>

  • Result on the web

    <a href="https://academic.oup.com/mnras/article-abstract/488/2/1917/5521914" target="_blank" >https://academic.oup.com/mnras/article-abstract/488/2/1917/5521914</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1093/mnras/stz1728" target="_blank" >10.1093/mnras/stz1728</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Powerful AGN jets and unbalanced cooling in the hot atmosphere of IC 4296

  • Original language description

    We present new Karl G. Jansky Very Large Array (VLA, 1.5 GHz) radio data for the giant elliptical galaxy IC 4296, supported by archival radio, X-ray (Chandra, XMMNewton) and optical (SOAR, HST) observations. The galaxy hosts powerful radio jets piercing through the inner hot X-ray emitting atmosphere, depositing most of the energy into the ambient intra-cluster medium (ICM). Whereas the radio surface brightness of the A configuration image is consistent with a Fanaroff-Riley Class I (FR I) system, the D configuration image shows two bright, relative to the central region, large (160 kpc diameter), well-defined lobes, previously reported by Killeen et al., at a projected distance r 230 kpc. The XMM-Newton image reveals an X-ray cavity associated with one of the radio lobes. The total enthalpy of the radio lobes is 7 × 1059 erg and the mechanical power output of the jets is 1044 erg s-1 . The jets are mildly curved and possibly re-brightened by the relative motion of the galaxy and the ICM. The lobes display sharp edges, suggesting the presence of bow shocks, which would indicate that they are expanding supersonically. The central entropy and cooling time of the X-ray gas are unusually low and the nucleus hosts a warm Ha+[N ii] nebula and a cold molecular CO disk. Because most of the energy of the jets is deposited far from the nucleus, the atmosphere of the galaxy continues to cool, apparently feeding the central supermassive black hole and powering the jet activity.

  • 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

  • Continuities

    S - Specificky vyzkum na vysokych skolach<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2019

  • 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, MALDEN, WILEY

  • ISSN

    0035-8711

  • e-ISSN

    1365-2966

  • Volume of the periodical

    488

  • Issue of the periodical within the volume

    2

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    9

  • Pages from-to

    1917-1925

  • UT code for WoS article

    000482332500028

  • EID of the result in the Scopus database

    2-s2.0-85074517935