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  • Olofsson, Hans,1952Chalmers tekniska högskola,Chalmers University of Technology,Chalmers Univ Technol, Dept Space Earth & Environm, Onsala Space Observ, S-43992 Onsala, Sweden (author)

HD 101584: circumstellar characteristics and evolutionary status

  • Article/chapterEnglish2019

Publisher, publication year, extent ...

  • 2019-03-25
  • EDP Sciences,2019
  • electronicrdacarrier

Numbers

  • LIBRIS-ID:oai:research.chalmers.se:c3527dc8-8a65-4e71-94f1-7f13ff17f3ef
  • https://research.chalmers.se/publication/513752URI
  • https://doi.org/10.1051/0004-6361/201834897DOI
  • https://research.chalmers.se/publication/509515URI
  • https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-381122URI

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  • Language:English
  • Summary in:English

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  • Subject category:art swepub-publicationtype
  • Subject category:ref swepub-contenttype

Notes

  • Context. There is growing evidence that red giant evolution is often affected by an interplay with a nearby companion, in some cases taking the form of a common-envelope evolution. Aims. We have performed a study of the characteristics of the circumstellar environment of the binary object HD 101584, that provides information on a likely evolutionary scenario. Methods. We have obtained and analysed ALMA observations, complemented with observations using APEX, of a large number of molecular lines. An analysis of the spectral energy distribution has also been performed. Results. Emissions from 12 molecular species (not counting isotopologues) have been observed, and most of them mapped with angular resolutions in the range 0 ''.1-0 ''.6. Four circumstellar components are identified: (i) a central compact source of size approximate to 0 ''.15, (ii) an expanding equatorial density enhancement (a flattened density distribution in the plane of the orbit) of size approximate to 3 '', (iii) a bipolar high-velocity outflow (approximate to 150 km s(-1)), and (iv) an hourglass structure. The outflow is directed almost along the line of sight. There is evidence of a second bipolar outflow. The mass of the circumstellar gas is approximate to 0.5 [D/1 kpc](2) M-circle dot, about half of it lies in the equatorial density enhancement. The dust mass is approximate to 0.01 [D/1 kpc](2) M-circle dot, and a substantial fraction of this is in the form of large-sized, up to 1 mm, grains. The estimated kinetic age of the outflow is approximate to 770 [D/1 kpc] yr. The kinetic energy and the scalar momentum of the accelerated gas are estimated to be 7 x 10(45) [D/1 kpc](2) erg and 10(39) [D/1 kpc](2) g cm s(-1), respectively. Conclusions. We provide good evidence that the binary system HD 101584 is in a post-common-envelope-evolution phase, that ended before a stellar merger. Isotope ratios combined with stellar mass estimates suggest that the primary star's evolution was terminated already on the first red giant branch (RGB). Most of the energy required to drive the outflowing gas was probably released when material fell towards the companion.

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  • Khouri, Theo,1985Chalmers tekniska högskola,Chalmers University of Technology,Chalmers Univ Technol, Dept Space Earth & Environm, Onsala Space Observ, S-43992 Onsala, Sweden(Swepub:cth)theok (author)
  • Maercker, Matthias,1979Chalmers tekniska högskola,Chalmers University of Technology,Chalmers Univ Technol, Dept Space Earth & Environm, Onsala Space Observ, S-43992 Onsala, Sweden,ESO, Karl Schwarzschild Str 2, D-85748 Garching, Germany(Swepub:cth)maercker (author)
  • Bergman, Per,1960Chalmers tekniska högskola,Chalmers University of Technology,Chalmers Univ Technol, Dept Space Earth & Environm, Onsala Space Observ, S-43992 Onsala, Sweden(Swepub:cth)pbergman (author)
  • Doan, LamUppsala universitet,Teoretisk astrofysik(Swepub:uu)lamdo353 (author)
  • Tafoya, D.National Astronomical Observatory of Japan,Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan (author)
  • Vlemmings, Wouter,1974Chalmers tekniska högskola,Chalmers University of Technology,Chalmers Univ Technol, Dept Space Earth & Environm, Onsala Space Observ, S-43992 Onsala, Sweden(Swepub:cth)wouterv (author)
  • Humphreys, E. M. L.European Southern Observatory (ESO) (author)
  • Lindqvist, Michael,1960Chalmers tekniska högskola,Chalmers University of Technology(Swepub:cth)mlq (author)
  • Nyman, L.European Southern Observatory (ESO),ESO, Alonso de Cordova 3107, Santiago, Chile (author)
  • Ramstedt, SofiaUppsala universitet,Teoretisk astrofysik(Swepub:uu)sofra336 (author)
  • Chalmers tekniska högskolaChalmers Univ Technol, Dept Space Earth & Environm, Onsala Space Observ, S-43992 Onsala, Sweden (creator_code:org_t)

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  • In:Astronomy and Astrophysics: EDP Sciences6230004-63611432-0746

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