TESS photometry of the nova eruption in V606 Vul: asymmetric photosphere and multiple ejections?
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| Format: | Preprint |
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2023
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| author | Sokolovsky, Kirill V. Aydi, Elias Malanchev, Konstantin Burke, Colin J. Mukai, Koji Sokoloski, Jennifer L. Metzger, Brian D. Atapin, Kirill E. Belinski, Aleksandre A. Chen, Yu-Ching Chomiuk, Laura Dubovsky, Pavol A. Faucher-Giguere, Claude-Andre Hounsell, Rebekah A. Ikonnikova, Natalia P. Lander, Vsevolod Yu. Li, Junyao Linford, Justin D. Mioduszewski, Amy J. Molina, Isabella Munari, Ulisse Potanin, Sergey A. Quimby, Robert M. Rupen, Michael P. Scaringi, Simone Shatsky, Nicolai I. Shen, Yue Steinberg, Elad Stone, Zachary Tatarnikov, Andrey M. Vurm, Indrek Williams, Montana N. Azcona, Antonio Agudo Boyd, David Bean, Stewart Braunwarth, Horst Blackwell, John Bolzoni, Simone Casas, Ricard Fernandez, David Cejudo Dubois, Franky Foster, James Farfan, Rafael Galdies, Charles Hodge, John Gallego, Jose Prieto Lane, David J. Larsson, Magnus Lindner, Peter Logie, Ludwig Mantero, Andrea Aimar, Mario Morales Menzies, Kenneth Nakonechny, Keith Philpot, Jerry Filho, Antonio Padilla Ramey, Brian Rau, Steve Reina, Esteban Romanov, Filipp D. Ruocco, Nello Shears, Jeremy Serreau, Marc Schmidt, Richard Solomonov, Yuri Tracy, Bob Tulloch, Gord Tomlin, Ray Tordai, Tamas Vanaverbeke, Siegfried Wenzel, Klaus Maitan, Alessandro Moretti, Stefano |
| author_facet | Sokolovsky, Kirill V. Aydi, Elias Malanchev, Konstantin Burke, Colin J. Mukai, Koji Sokoloski, Jennifer L. Metzger, Brian D. Atapin, Kirill E. Belinski, Aleksandre A. Chen, Yu-Ching Chomiuk, Laura Dubovsky, Pavol A. Faucher-Giguere, Claude-Andre Hounsell, Rebekah A. Ikonnikova, Natalia P. Lander, Vsevolod Yu. Li, Junyao Linford, Justin D. Mioduszewski, Amy J. Molina, Isabella Munari, Ulisse Potanin, Sergey A. Quimby, Robert M. Rupen, Michael P. Scaringi, Simone Shatsky, Nicolai I. Shen, Yue Steinberg, Elad Stone, Zachary Tatarnikov, Andrey M. Vurm, Indrek Williams, Montana N. Azcona, Antonio Agudo Boyd, David Bean, Stewart Braunwarth, Horst Blackwell, John Bolzoni, Simone Casas, Ricard Fernandez, David Cejudo Dubois, Franky Foster, James Farfan, Rafael Galdies, Charles Hodge, John Gallego, Jose Prieto Lane, David J. Larsson, Magnus Lindner, Peter Logie, Ludwig Mantero, Andrea Aimar, Mario Morales Menzies, Kenneth Nakonechny, Keith Philpot, Jerry Filho, Antonio Padilla Ramey, Brian Rau, Steve Reina, Esteban Romanov, Filipp D. Ruocco, Nello Shears, Jeremy Serreau, Marc Schmidt, Richard Solomonov, Yuri Tracy, Bob Tulloch, Gord Tomlin, Ray Tordai, Tamas Vanaverbeke, Siegfried Wenzel, Klaus Maitan, Alessandro Moretti, Stefano |
| contents | Lightcurves of many classical novae deviate from the canonical "fast rise - smooth decline" pattern and display complex variability behavior. We present the first TESS-space-photometry-based investigation of this phenomenon. We use Sector 41 full-frame images to extract a lightcurve of the slow Galactic nova V606 Vul that erupted nine days prior to the start of the TESS observations. The lightcurve covers the first of two major peaks of V606 Vul that was reached 19 days after the start of the eruption. The nova reached its brightest visual magnitude V=9.9 in its second peak 64 days after the eruption onset, following the completion of Sector 41 observations. To increase the confidence level of the extracted lightcurve, we performed the analysis using four different codes implementing the aperture photometry (Lightkurve, VaST) and image subtraction (TESSreduce, tequila_shots) and find good agreement between them. We performed ground-based photometric and spectroscopic monitoring to complement the TESS data. The TESS lightcurve reveals two features: periodic variations (0.12771 d, 0.01 mag average peak-to-peak amplitude) that disappeared when the source was within 1 mag of peak optical brightness and a series of isolated mini-flares (with peak-to-peak amplitudes of up to 0.5 mag) appearing at seemingly random times. We interpret the periodic variations as the result of azimuthal asymmetry of the photosphere engulfing the nova-hosting binary that was distorted by and rotating with the binary. Whereas we use spectra to associate the two major peaks in the nova lightcurve with distinct episodes of mass ejection, the origin of mini-flares remains elusive. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2311_04903 |
| institution | arXiv |
| publishDate | 2023 |
| record_format | arxiv |
| spellingShingle | TESS photometry of the nova eruption in V606 Vul: asymmetric photosphere and multiple ejections? Sokolovsky, Kirill V. Aydi, Elias Malanchev, Konstantin Burke, Colin J. Mukai, Koji Sokoloski, Jennifer L. Metzger, Brian D. Atapin, Kirill E. Belinski, Aleksandre A. Chen, Yu-Ching Chomiuk, Laura Dubovsky, Pavol A. Faucher-Giguere, Claude-Andre Hounsell, Rebekah A. Ikonnikova, Natalia P. Lander, Vsevolod Yu. Li, Junyao Linford, Justin D. Mioduszewski, Amy J. Molina, Isabella Munari, Ulisse Potanin, Sergey A. Quimby, Robert M. Rupen, Michael P. Scaringi, Simone Shatsky, Nicolai I. Shen, Yue Steinberg, Elad Stone, Zachary Tatarnikov, Andrey M. Vurm, Indrek Williams, Montana N. Azcona, Antonio Agudo Boyd, David Bean, Stewart Braunwarth, Horst Blackwell, John Bolzoni, Simone Casas, Ricard Fernandez, David Cejudo Dubois, Franky Foster, James Farfan, Rafael Galdies, Charles Hodge, John Gallego, Jose Prieto Lane, David J. Larsson, Magnus Lindner, Peter Logie, Ludwig Mantero, Andrea Aimar, Mario Morales Menzies, Kenneth Nakonechny, Keith Philpot, Jerry Filho, Antonio Padilla Ramey, Brian Rau, Steve Reina, Esteban Romanov, Filipp D. Ruocco, Nello Shears, Jeremy Serreau, Marc Schmidt, Richard Solomonov, Yuri Tracy, Bob Tulloch, Gord Tomlin, Ray Tordai, Tamas Vanaverbeke, Siegfried Wenzel, Klaus Maitan, Alessandro Moretti, Stefano Solar and Stellar Astrophysics High Energy Astrophysical Phenomena Lightcurves of many classical novae deviate from the canonical "fast rise - smooth decline" pattern and display complex variability behavior. We present the first TESS-space-photometry-based investigation of this phenomenon. We use Sector 41 full-frame images to extract a lightcurve of the slow Galactic nova V606 Vul that erupted nine days prior to the start of the TESS observations. The lightcurve covers the first of two major peaks of V606 Vul that was reached 19 days after the start of the eruption. The nova reached its brightest visual magnitude V=9.9 in its second peak 64 days after the eruption onset, following the completion of Sector 41 observations. To increase the confidence level of the extracted lightcurve, we performed the analysis using four different codes implementing the aperture photometry (Lightkurve, VaST) and image subtraction (TESSreduce, tequila_shots) and find good agreement between them. We performed ground-based photometric and spectroscopic monitoring to complement the TESS data. The TESS lightcurve reveals two features: periodic variations (0.12771 d, 0.01 mag average peak-to-peak amplitude) that disappeared when the source was within 1 mag of peak optical brightness and a series of isolated mini-flares (with peak-to-peak amplitudes of up to 0.5 mag) appearing at seemingly random times. We interpret the periodic variations as the result of azimuthal asymmetry of the photosphere engulfing the nova-hosting binary that was distorted by and rotating with the binary. Whereas we use spectra to associate the two major peaks in the nova lightcurve with distinct episodes of mass ejection, the origin of mini-flares remains elusive. |
| title | TESS photometry of the nova eruption in V606 Vul: asymmetric photosphere and multiple ejections? |
| topic | Solar and Stellar Astrophysics High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2311.04903 |