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Evidence for the Disruption of a Planetary System During the Formation of the Helix Nebula

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A90259%2F23%3A00583717" target="_blank" >RIV/67985815:90259/23:00583717 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.3847/1538-3881/ac9d90" target="_blank" >https://doi.org/10.3847/1538-3881/ac9d90</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.3847/1538-3881/ac9d90" target="_blank" >10.3847/1538-3881/ac9d90</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Evidence for the Disruption of a Planetary System During the Formation of the Helix Nebula

  • Original language description

    We combine infrared (Stratospheric Observatory for Infrared Astronomy, Spitzer, Herschel) and millimeter (Atacama Large Millimeter/submillimeter Array) observations of the system to determine the origin of this excess using multiwavelength imaging and radiative transfer modeling. We find the data are incompatible with a compact remnant planetesimal belt or post-AGB disk, and conclude the dust most likely originates from deposition by a cometary cloud. The measured dust mass, and lifetime of the constituent grains, implies disruption of several thousand Hale-Bopp equivalent comets per year to fuel the observed excess emission around the Helix Nebula's white dwarf.

  • 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

Others

  • Publication year

    2023

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Astronomical Journal

  • ISSN

    0004-6256

  • e-ISSN

    1538-3881

  • Volume of the periodical

    165

  • Issue of the periodical within the volume

    1

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    11

  • Pages from-to

    22

  • UT code for WoS article

    000908816800001

  • EID of the result in the Scopus database

    2-s2.0-85145290319