Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.

Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): Scattered light detection of a possible disk wind in RY Tau

Autor: P.-G. Valegård, C. Ginski, C. Dominik, J. Bae, M. Benisty, T. Birnstiel, S. Facchini, A. Garufi, M. Hogerheijde, R. G. van Holstein, M. Langlois, C. F. Manara, P. Pinilla, Ch. Rab, Á. Ribas, L. B. F. M. Waters, J. Williams

Publikováno v: Astronomy and Astrophysics, 668:A25. EDP Sciences
Astronomy & Astrophysics, 668, 1-10
Astronomy & Astrophysics, 668, pp. 1-10
Astronomy & Astrophysics, 668:A25

Disk winds are an important mechanism for accretion and disk evolution around young stars. The accreting intermediate-mass T-Tauri star RY Tau has an active jet and a previously known disk wind. Archival optical and new near-infrared observations of

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::08f0f13ce787760b57008d7b80e960e8
http://arxiv.org/abs/2209.01969

An Event Horizon Imager (EHI) Mission Concept Utilizing Medium Earth Orbit Sub-mm Interferometry*

Autor: V KUDRIASHOV, M MARTIN-NEIRA, F ROELOFS, H FALCKE, C BRINKERINK, A BARYSHEV, M HOGERHEIJDE, A YOUNG, H POURSHAGHAGHI, M KLEIN-WOLT, M MOSCIBRODZKA, J DAVELAAR, I BARAT, B DUESMANN, V VALENTA, ARMENGOL J M PERDIGUES, D DE WILDE, IGLESIAS P MARTIN, N ALAGHA, DER VORST M VAN

Publikováno v: Chinese Journal of Space Science. 41:211-233

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::3bebc80e8e2d36f9a6927c7b775d51bd
https://doi.org/10.3724/sp.j.0254-6124.2021.0202

Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.

The disk of FU Orionis viewed with MATISSE/VLTI

Autor: F. Lykou, P. Ábrahám, L. Chen, J. Varga, Á. Kóspál, A. Matter, M. Siwak, Zs. M. Szabó, Z. Zhu, H. B. Liu, B. Lopez, F. Allouche, J.-C. Augereau, P. Berio, P. Cruzalèbes, C. Dominik, Th. Henning, K.-H. Hofmann, M. Hogerheijde, W. J. Jaffe, E. Kokoulina, S. Lagarde, A. Meilland, F. Millour, E. Pantin, R. Petrov, S. Robbe-Dubois, D. Schertl, M. Scheuck, R. van Boekel, L. B. F. M. Waters, G. Weigelt, S. Wolf

Publikováno v: Astronomy & Astrophysics, 663:A86
Astronomy & Astrophysics, 663:A86. EDP Sciences
Astronomy & Astrophysics, 663, pp. 1-17
Astronomy & Astrophysics, 663, 1-17
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 663, ⟨10.1051/0004-6361/202142788⟩
Astronomy & Astrophysics

The disk of FU Orionis is marginally resolved with MATISSE, suggesting that the region emitting in the thermal infrared is rather compact. An upper limit of $\sim1.3\pm0.1$ mas (in $L$) can be given for the diameter of the disk region probed in the $

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::71eb1db65d09c3fb19a2f898f72d1895
https://doi.org/10.1051/0004-6361/202142788