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The infrared K-band identification of the DSO/G2 source from VLT and Keck data

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F14%3A00429558" target="_blank" >RIV/67985815:_____/14:00429558 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1017/S1743921314000726" target="_blank" >http://dx.doi.org/10.1017/S1743921314000726</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1017/S1743921314000726" target="_blank" >10.1017/S1743921314000726</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    The infrared K-band identification of the DSO/G2 source from VLT and Keck data

  • Original language description

    A fast moving infrared excess source (G2) which is widely interpreted as a core-less gas and dust cloud approaches Sagittarius A* (Sgr A*) on a presumably elliptical orbit. VLT Ks -band and Keck K'-band data result in clear continuum identifications and proper motions of this ˜19 m Dusty S-cluster Object (DSO). In 2002-2007 it is confused with the star S63, but free of confusion again since 2007. Its near-infrared (NIR) colors and a comparison to other sources in the field speak in favor of the DSO being an IR excess star with photospheric continuum emission at 2 microns than a core-less gas and dust cloud. We also find very compact L'-band emission (<0.1") contrasted by the reported extended (0.03" up to ˜0.2" for the tail) Brgamma emission. The presence of a star will change the expected accretion phenomena, since a stellar Roche lobe may retain a fraction of the material during and after the peri-bothron passage.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2014

  • Confidentiality

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

Data specific for result type

  • Article name in the collection

    The Galactic center: Feeding and Feedback in a Normal Galactic Nucleus

  • ISBN

    9781107044616

  • ISSN

    1743-9213

  • e-ISSN

  • Number of pages

    5

  • Pages from-to

    269-273

  • Publisher name

    Cambridge University Press

  • Place of publication

    Cambridge

  • Event location

    Santa Fe

  • Event date

    Sep 30, 2013

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article

    000450812600064