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COMP2CAT: hunting compact double radio sources in the local Universe

Identifikátory výsledku

  • Kód výsledku v IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F19%3A00110294" target="_blank" >RIV/00216224:14310/19:00110294 - isvavai.cz</a>

  • Výsledek na webu

    <a href="https://arxiv.org/abs/1905.02212" target="_blank" >https://arxiv.org/abs/1905.02212</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/201935104" target="_blank" >10.1051/0004-6361/201935104</a>

Alternativní jazyky

  • Jazyk výsledku

    angličtina

  • Název v původním jazyce

    COMP2CAT: hunting compact double radio sources in the local Universe

  • Popis výsledku v původním jazyce

    We present a catalog of compact double radio galaxies (hereafter COMP2CAT) listing 43 edge-brightened radio sources whose projected linear size does not exceed 60 kpc, the typical size of their host galaxies. This is the fifth in a series of radio source catalogs recently created, namely: FRICAT, FRIICAT, FR0CAT, and WATCAT, each of which focuses on a different class of radio galaxies. The main aim of our analysis is to attain a better understanding of sources with intermediate morphologies between FR IIs and FR 0s. COMP2CAT sources were selected from an existing catalog of radio sources based on NVSS, FIRST and SDSS observations because they have (i) edge-brightened morphologies typical of FR IIs, (ii) redshifts z &lt; 0.15, and (iii) projected linear sizes smaller than 60 kpc. With radio luminosities at 1.4 GHz 10(38) less than or similar to L-1.4 less than or similar to 10(41) erg s(-1), COMP2CAT sources appear as the low radio luminosity tail of FR IIs. However, their host galaxies are indistinguishable from those of large-scale radio sources: they are luminous (-21 greater than or similar to M-r greater than or similar to -24), red, early-type galaxies with black hole masses in the range 10(7.5) less than or similar to M-BH less than or similar to 10(9.5) M-circle dot. Moreover, all but one of the COMP2CAT sources are optically classifiable as low-excitation radio galaxies, in agreement with being the low radio luminosity tail of FR Is and FR IIs. This catalog of compact double sources, which is similar to 47% complete at z &lt; 0.15, can potentially be used to clarify the role of compact double sources in the general evolutionary scheme of radio galaxies.

  • Název v anglickém jazyce

    COMP2CAT: hunting compact double radio sources in the local Universe

  • Popis výsledku anglicky

    We present a catalog of compact double radio galaxies (hereafter COMP2CAT) listing 43 edge-brightened radio sources whose projected linear size does not exceed 60 kpc, the typical size of their host galaxies. This is the fifth in a series of radio source catalogs recently created, namely: FRICAT, FRIICAT, FR0CAT, and WATCAT, each of which focuses on a different class of radio galaxies. The main aim of our analysis is to attain a better understanding of sources with intermediate morphologies between FR IIs and FR 0s. COMP2CAT sources were selected from an existing catalog of radio sources based on NVSS, FIRST and SDSS observations because they have (i) edge-brightened morphologies typical of FR IIs, (ii) redshifts z &lt; 0.15, and (iii) projected linear sizes smaller than 60 kpc. With radio luminosities at 1.4 GHz 10(38) less than or similar to L-1.4 less than or similar to 10(41) erg s(-1), COMP2CAT sources appear as the low radio luminosity tail of FR IIs. However, their host galaxies are indistinguishable from those of large-scale radio sources: they are luminous (-21 greater than or similar to M-r greater than or similar to -24), red, early-type galaxies with black hole masses in the range 10(7.5) less than or similar to M-BH less than or similar to 10(9.5) M-circle dot. Moreover, all but one of the COMP2CAT sources are optically classifiable as low-excitation radio galaxies, in agreement with being the low radio luminosity tail of FR Is and FR IIs. This catalog of compact double sources, which is similar to 47% complete at z &lt; 0.15, can potentially be used to clarify the role of compact double sources in the general evolutionary scheme of radio galaxies.

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

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Ostatní

  • Rok uplatnění

    2019

  • Kód důvěrnosti údajů

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

Údaje specifické pro druh výsledku

  • Název periodika

    ASTRONOMY & ASTROPHYSICS

  • ISSN

    1432-0746

  • e-ISSN

  • Svazek periodika

    627

  • Číslo periodika v rámci svazku

    JUL 8 2019

  • Stát vydavatele periodika

    FR - Francouzská republika

  • Počet stran výsledku

    21

  • Strana od-do

    1-21

  • Kód UT WoS článku

    000474334400001

  • EID výsledku v databázi Scopus

    2-s2.0-85069438256