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Colliding interstellar bubbles in the direction of l=54 degrees

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F16%3A00094217" target="_blank" >RIV/00216224:14310/16:00094217 - isvavai.cz</a>

  • Alternative codes found

    RIV/67985815:_____/16:00471443

  • Result on the web

    <a href="http://dx.doi.org/10.1051/0004-6361/201527897" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201527897</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/201527897" target="_blank" >10.1051/0004-6361/201527897</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Colliding interstellar bubbles in the direction of l=54 degrees

  • Original language description

    Context. Interstellar bubbles are structures in the interstellar medium with diameters of a few to tens of parsecs. Their progenitors are stellar winds, intense radiation of massive stars, or supernova explosions. Star formation and young stellar objects are commonly associated with these structures. Aims. We compare infrared observations of bubbles N115, N116 and N117 with atomic, molecular and ionized gas in this region. While determining the dynamical properties of the bubbles, we also look into their ambient environment to understand their formation in a wider context. Methods. To find bubbles in HI (Very Large Array Galactic Plane Survey) and CO data (Galactic Ring Survey), we used the images from the Galactic Legacy Infrared Mid-Plane Survey. We manually constructed masks based on the appearance of the bubbles in the IR images and applied them to the HI and CO data.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

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

Others

  • Publication year

    2016

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    ASTRONOMY & ASTROPHYSICS

  • ISSN

    1432-0746

  • e-ISSN

  • Volume of the periodical

    595

  • Issue of the periodical within the volume

    November

  • Country of publishing house

    FR - FRANCE

  • Number of pages

    9

  • Pages from-to

    "A49"-"A57"

  • UT code for WoS article

    000388573500017

  • EID of the result in the Scopus database