Park, Sunkyung and Kóspál, Ágnes and Cruz-Saenz de Miera, Fernando and Siwak, Michal and Dróżdż, Marek and Ignácz, Bernadett and Jaffe, T. Daniel and Könyves-Tóth, Réka and Kriskovics, Levente and Pál, András and Szabó, Zsófia Marianna (2021) V899 Mon: A Peculiar Eruptive Young Star Close to the End of Its Outburst. ASTROPHYSICAL JOURNAL, 923 (2). No.-171. ISSN 1538-4357
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Official URL: https://doi.org/10.3847/1538-4357/ac29c4
| Item Type: | Article |
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| Additional Information: | Funding Agency and Grant Number: Mt. Cuba Astronomical Foundation; US National Science Foundation [AST-1229522, AST-1702267]; McDonald Observatory of the University of Texas at Austin; Korean GMT Project of KASI; Gemini Observatory; K-GMT Science Program of the Korea Astronomy and Space Science Institute (KASI) [PID: GS-2020B-Q-218]; European Research Council (ERC) under the European Union [716155]; National Research, Development and Innovation Office (NKFIH), Hungary - European Union [GINOP 2.3.2-15-201600033]; New National Excellence Program of the Ministry for Innovation and Technology from the source of the National Research, Development and Innovation Fund [UNKP-20-2]; Bolyai Janos Research Scholarship of the Hungarian Academy of Sciences; Hungarian National Research, Development and Innovation Office [NKFIH PD-134784] Funding text: This work used the Immersion Grating Infrared Spectrometer (IGRINS) that was developed under a collaboration between the University of Texas at Austin and the Korea Astronomy and Space Science Institute (KASI) with the financial support of the Mt. Cuba Astronomical Foundation, the US National Science Foundation under grants AST-1229522 and AST-1702267, the McDonald Observatory of the University of Texas at Austin, the Korean GMT Project of KASI, and Gemini Observatory. This work was supported by the K-GMT Science Program (PID: GS-2020B-Q-218) of the Korea Astronomy and Space Science Institute (KASI). We gratefully acknowledge the work of the observers, Robert Szakats, Eda Sonbas, and Huseyin Er. This project has received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program under grant agreement No. 716155 (SACCRED) and the "Transient Astrophysical Objects" GINOP 2.3.2-15-201600033 project of the National Research, Development and Innovation Office (NKFIH), Hungary, funded by the European Union. Zs.M.Sz is supported by the UNKP-20-2 New National Excellence Program of the Ministry for Innovation and Technology from the source of the National Research, Development and Innovation Fund. L.K. is supported by the Bolyai Janos Research Scholarship of the Hungarian Academy of Sciences. L.K. acknowledges the financial support of Hungarian National Research, Development and Innovation Office grant NKFIH PD-134784. This paper uses observations made at the South African Astronomical Observatory (SAAO) and the Mount Suhora Astronomical Observatory. |
| Subjects: | Q Science / természettudomány > QB Astronomy, Astrophysics / csillagászat, asztrofizika |
| SWORD Depositor: | MTMT SWORD |
| Depositing User: | MTMT SWORD |
| Date Deposited: | 27 Sep 2022 11:39 |
| Last Modified: | 27 Sep 2022 11:39 |
| URI: | http://real.mtak.hu/id/eprint/150069 |
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