In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 49, no. 2
Z. Garai
Details:
Year, pages: 2019, 352 - 354
Language: eng
Keywords:
planets and satellites: general, planet-star interactions, scattering
Original source URL: http://www.astro.sk/caosp/Eedition/Abstracts/2019/Vol_49/No_2/pp352-354_abstract.html
About article:
The Kepler object KOI 2700b was discovered recently as the second exoplanet with a comet-like dusty tail. Previously, we aimed at verifying the disintegrating-planet scenario of KOI 2700b by modeling its light curve and to put constraints on various tail and planet properties, as was done in the case of KIC 12557548b. Here, we describe an improved tail model with five free parameters and its application in the case of ≳mma-alumina 1 micron grains.
How to cite:
ISO 690:
Garai, Z. 2019. Analysis of KOI 2700b: the second exoplanet with a comet-like dusty tail. An improved tail model. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 49, no.2, pp. 352-354. 1335-1842.
APA:
Garai, Z. (2019). Analysis of KOI 2700b: the second exoplanet with a comet-like dusty tail. An improved tail model. Contributions of the Astronomical Observatory Skalnaté Pleso, 49(2), 352-354. 1335-1842.
About edition:
Publisher: Astronomical Institute, Slovak Academy of Sciences
Published: 1. 5. 2019
Rights:
