E-viri
Odprti dostop
-
Sokolovsky, Kirill V; Aydi, Elias; Malanchev, Konstantin; Burke, Colin J; Mukai, Koji; Sokoloski, J L; Metzger, Brian D; Atapin, Kirill E; Belinski, Aleksandre A; Yu-Ching, Chen; Chomiuk, Laura; Dubovsky, Pavol A; Claude-Andre Faucher-Giguere; Hounsell, Rebekah A; Ikonnikova, Natalia P; Vsevolod Yu Lander; 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; Antonio Agudo Azcona; Boyd, David; Bean, Stewart; Braunwarth, Horst; Blackwell, John; Bolzoni, Simone; Casas, Ricard; David Cejudo Fernandez; Dubois, Franky; Foster, James; Farfan, Rafael; Galdies, Charles; Hodge, John; Jose Prieto Gallego; Lane, David J; Larsson, Magnus; Lindner, Peter; Logie, Ludwig; Mantero, Andrea; Mario Morales Aimar; Menzies, Kenneth; Nakonechny, Keith; Philpot, Jerry; Antonio Padilla Filho; 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
arXiv.org, 11/2023Paper, Journal Article
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 TESS 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 (0.12771d, 0.01mag average peak-to-peak amplitude) that disappeared when the source was within 1mag of peak optical brightness and a series of isolated mini-flares (with peak-to-peak amplitudes of up to 0.5mag) 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.
Avtor
![loading ... loading ...](themes/default/img/ajax-loading.gif)
Vnos na polico
Trajna povezava
- URL:
Faktor vpliva
Dostop do baze podatkov JCR je dovoljen samo uporabnikom iz Slovenije. Vaš trenutni IP-naslov ni na seznamu dovoljenih za dostop, zato je potrebna avtentikacija z ustreznim računom AAI.
Leto | Faktor vpliva | Izdaja | Kategorija | Razvrstitev | ||||
---|---|---|---|---|---|---|---|---|
JCR | SNIP | JCR | SNIP | JCR | SNIP | JCR | SNIP |
Baze podatkov, v katerih je revija indeksirana
Ime baze podatkov | Področje | Leto |
---|
Povezave do osebnih bibliografij avtorjev | Povezave do podatkov o raziskovalcih v sistemu SICRIS |
---|
Vir: Osebne bibliografije
in: SICRIS
To gradivo vam je dostopno v celotnem besedilu. Če kljub temu želite naročiti gradivo, kliknite gumb Nadaljuj.