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Sökning: WFRF:(Drevon C. A.) > The extended atmosp...

LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00010238naa a2201057 4500
001oai:DiVA.org:uu-470462
003SwePub
008220328s2022 | |||||||||||000 ||eng|
024a https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-4704622 URI
024a https://doi.org/10.1051/0004-6361/2021425142 DOI
040 a (SwePub)uu
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a art2 swepub-publicationtype
100a Chiavassa, A.u Univ Cote dAzur, CNRS, Observ Cote dAzur, CS 34229, F-34229 Nice, France.;European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany.;Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85741 Garching, Germany.4 aut
2451 0a The extended atmosphere and circumstellar environment of the cool evolved star VX Sagittarii as seen by MATISSE star
264 c 2022-02-21
264 1b EDP Sciences,c 2022
338 a electronic2 rdacarrier
520 a Context. VX Sgr is a cool, evolved, and luminous red star whose stellar parameters are difficult to determine, which affects its classification.Aims. We aim to spatially resolve the photospheric extent as well as the circumstellar environment.Methods. We used interferometric observations obtained with the MATISSE instrument in the L (3-4 mu m), M (4.5-5 mu m), and N (8-13 mu m) bands. We reconstructed monochromatic images using the MIRA software. We used 3D radiation-hydrodynamics simulations carried out with (COBOLD)-B-5 and a uniform disc model to estimate the apparent diameter and interpret the stellar surface structures. Moreover, we employed the radiative transfer codes OPTIM3D and RADMC3D to compute the spectral energy distribution for the L, M, and N bands, respectively.Results. MATISSE observations unveil, for the first time, the morphology of VX Sgr across the L, M, and N bands. The reconstructed images show a complex morphology with brighter areas whose characteristics depend on the wavelength probed. We measured the angular diameter as a function of the wavelength and showed that the photospheric extent in the L and M bands depends on the opacity through the atmosphere. In addition to this, we also concluded that the observed photospheric inhomogeneities can be interpreted as convection-related surface structures. The comparison in the N band yielded a qualitative agreement between the N-band spectrum and simple dust radiative transfer simulations. However, it is not possible to firmly conclude on the interpretation of the current data because of the difficulty in constraing the model parameters using the limited accuracy of our absolute flux calibration.Conclusions. MATISSE observations and the derived reconstructed images unveil the appearance of VX Sgr's stellar surface and circumstellar environment across a very large spectral domain for the first time.
650 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
653 a stars
653 a atmospheres
653 a late-type
653 a individual
653 a VX Sgr
653 a techniques
653 a interferometric
653 a infrared
653 a imaging
700a Kravchenko, K.u Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany.4 aut
700a Montarges, M.u Univ Paris, Observ Paris, Sorbonne Univ, CNRS,LESIA,Univ PSL, 5 Pl Jules Janssen, F-92195 Meudon, France.4 aut
700a Millour, F.u Univ Cote dAzur, CNRS, Observ Cote dAzur, CS 34229, F-34229 Nice, France.4 aut
700a Matter, A.u Univ Cote dAzur, CNRS, Observ Cote dAzur, CS 34229, F-34229 Nice, France.4 aut
700a Freytag, Bernd,c Dr.u Uppsala universitet,Teoretisk astrofysik4 aut0 (Swepub:uu)befre677
700a Wittkowski, M.u European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany.4 aut
700a Hocde, Vu Polish Acad Sci, Nicolaus Copernicus Astron Ctr, Bartycka 18, PL-00716 Warsaw, Poland.4 aut
700a Cruzalebes, P.u Univ Cote dAzur, CNRS, Observ Cote dAzur, CS 34229, F-34229 Nice, France.4 aut
700a Allouche, F.u Univ Cote dAzur, CNRS, Observ Cote dAzur, CS 34229, F-34229 Nice, France.4 aut
700a Lopez, B.u Univ Cote dAzur, CNRS, Observ Cote dAzur, CS 34229, F-34229 Nice, France.4 aut
700a Lagarde, S.u Univ Cote dAzur, CNRS, Observ Cote dAzur, CS 34229, F-34229 Nice, France.4 aut
700a Petrov, R. G.u Univ Cote dAzur, CNRS, Observ Cote dAzur, CS 34229, F-34229 Nice, France.4 aut
700a Meilland, A.u Univ Cote dAzur, CNRS, Observ Cote dAzur, CS 34229, F-34229 Nice, France.4 aut
700a Robbe-Dubois, S.u Univ Cote dAzur, CNRS, Observ Cote dAzur, CS 34229, F-34229 Nice, France.4 aut
700a Hofmann, K-Hu Max Planck Inst Radioastron, Auf Hugel 69, D-53121 Bonn, Germany.4 aut
700a Weigelt, G.u Max Planck Inst Radioastron, Auf Hugel 69, D-53121 Bonn, Germany.4 aut
700a Berio, P.u Univ Cote dAzur, CNRS, Observ Cote dAzur, CS 34229, F-34229 Nice, France.4 aut
700a Bendjoya, P.u Univ Cote dAzur, CNRS, Observ Cote dAzur, CS 34229, F-34229 Nice, France.4 aut
700a Bettonvil, F.u Leiden Univ, Leiden Observ, Niels Bohrweg 2, NL-2333 CA Leiden, Netherlands.4 aut
700a de Souza, A. Domicianou Univ Cote dAzur, CNRS, Observ Cote dAzur, CS 34229, F-34229 Nice, France.4 aut
700a Heininger, M.u Max Planck Inst Radioastron, Auf Hugel 69, D-53121 Bonn, Germany.4 aut
700a Henning, Thu Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany.4 aut
700a Isbell, J. W.u Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany.4 aut
700a Jaffe, W.u Leiden Univ, Leiden Observ, Niels Bohrweg 2, NL-2333 CA Leiden, Netherlands.4 aut
700a Labadie, L.u Univ Cologne, Phys Inst 1, Zupicher Str 77, D-50937 Cologne, Germany.4 aut
700a Lehmitz, M.u Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany.4 aut
700a Meisenheimer, K.u Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany.4 aut
700a Soulain, A.u Univ Grenoble Alpes, IPAG, CNRS, F-38000 Grenoble, France.4 aut
700a Varga, J.u Leiden Univ, Leiden Observ, Niels Bohrweg 2, NL-2333 CA Leiden, Netherlands.;Eotvos Lorand Res Network ELKH, Konkoly Observ, Res Ctr Astron & Earth Sci, Konkoly Thege Miklos Ut 15-17, H-1121 Budapest, Hungary.4 aut
700a Augereau, J-Cu Univ Grenoble Alpes, IPAG, CNRS, F-38000 Grenoble, France.4 aut
700a van Boekel, R.u Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany.4 aut
700a Burtscher, L.u Leiden Univ, Leiden Observ, Niels Bohrweg 2, NL-2333 CA Leiden, Netherlands.4 aut
700a Danchi, W. C.u NASA, Astrophys Div, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA.4 aut
700a Dominik, C.u Univ Amsterdam, Anton Pannekoek Inst Astron, Sci Pk 904, NL-1090 GE Amsterdam, Netherlands.4 aut
700a Drevon, J.u Univ Cote dAzur, CNRS, Observ Cote dAzur, CS 34229, F-34229 Nice, France.4 aut
700a Rosas, V. Gamezu Leiden Univ, Leiden Observ, Niels Bohrweg 2, NL-2333 CA Leiden, Netherlands.4 aut
700a Hogerheijde, M. R.u Leiden Univ, Leiden Observ, Niels Bohrweg 2, NL-2333 CA Leiden, Netherlands.;Univ Amsterdam, Anton Pannekoek Inst Astron, Sci Pk 904, NL-1090 GE Amsterdam, Netherlands.4 aut
700a Hron, J.u Univ Vienna, Dept Astrophys, Turkenschanzstr 17, A-1180 Vienna, Austria.4 aut
700a Klarmann, L.u Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany.4 aut
700a Kokoulina, E.u Univ Cote dAzur, CNRS, Observ Cote dAzur, CS 34229, F-34229 Nice, France.4 aut
700a Lagadec, E.u Univ Cote dAzur, CNRS, Observ Cote dAzur, CS 34229, F-34229 Nice, France.4 aut
700a Leftley, J.u Univ Cote dAzur, CNRS, Observ Cote dAzur, CS 34229, F-34229 Nice, France.4 aut
700a Mosoni, L.u Zselic Pk Stars, 064-2 Hrsz, H-7477 Zselickisfalud, Hungary.4 aut
700a Nardetto, N.u Univ Cote dAzur, CNRS, Observ Cote dAzur, CS 34229, F-34229 Nice, France.4 aut
700a Paladini, C.u European Southern Observ, Alonso de Cordova 3107,Casilla 19, Santiago 19001, Chile.4 aut
700a Pantin, E.u Univ Paris Saclay, Univ Paris Diderot, CNRS, CEA,AIM,Sorbonne Paris Cite, F-91191 Gif Sur Yvette, France.4 aut
700a Schertl, D.u Max Planck Inst Radioastron, Auf Hugel 69, D-53121 Bonn, Germany.4 aut
700a Stee, P.u Univ Cote dAzur, CNRS, Observ Cote dAzur, CS 34229, F-34229 Nice, France.4 aut
700a Szabados, L.u Eotvos Lorand Res Network ELKH, Konkoly Observ, Res Ctr Astron & Earth Sci, Konkoly Thege Miklos Ut 15-17, H-1121 Budapest, Hungary.;CSFK Lendulet Near Field Cosmol Res Grp, Budapest, Hungary.4 aut
700a Waters, R.u Radboud Univ Nijmegen, Inst Math Astrophys & Particle Phys, POB 9010,MC 62, NL-6500 GL Nijmegen, Netherlands.;SRON Netherlands Inst Space Res, Sorbonnelaan 2, NL-3584 CA Utrecht, Netherlands.4 aut
700a Wolf, S.u Univ Kiel, Inst Theoret Phys & Astrophys, Leibnizstr 15, D-24118 Kiel, Germany.4 aut
700a Yoffe, G.u Leiden Univ, Leiden Observ, Niels Bohrweg 2, NL-2333 CA Leiden, Netherlands.4 aut
710a Univ Cote dAzur, CNRS, Observ Cote dAzur, CS 34229, F-34229 Nice, France.;European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany.;Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85741 Garching, Germany.b Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany.4 org
773t Astronomy and Astrophysicsd : EDP Sciencesg 658q 658x 0004-6361x 1432-0746
856u https://doi.org/10.1051/0004-6361/202142514y Fulltext
856u https://uu.diva-portal.org/smash/get/diva2:1647691/FULLTEXT01.pdfx primaryx Raw objecty fulltext:print
856u http://arxiv.org/pdf/2112.10695
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-470462
8564 8u https://doi.org/10.1051/0004-6361/202142514

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