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相关论文: KIC 8462852: Transit of a Large Comet Family

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As revealed by its peculiar Kepler light curve, the enigmatic star KIC 8462852 undergoes short and deep flux dimmings at a priori unrelated epochs. It presents nonetheless all other characteristics of a quiet 1 Gyr old F3V star. These…

KIC8462852 is a completely-ordinary F3 main sequence star, except that the light curve from Kepler shows episodes of unique and inexplicable day-long dips with up to 20% dimming. Here, I provide a light curve of 1338 Johnson B-band…

太阳与恒星天体物理 · 物理学 2016-05-25 Bradley E. Schaefer

Over the duration of the Kepler mission, KIC8462852 was observed to undergo irregularly shaped, aperiodic dips in flux of up to $\sim 20$\%. The dipping activity can last for between 5 and 80 days. We characterize the object with…

We present the first good evidence for exocomet transits of a host star in continuum light in data from the Kepler mission. The Kepler star in question, KIC 3542116, is of spectral type F2V and is quite bright at K_p = 10. The transits have…

地球与行星天体物理 · 物理学 2018-01-24 S. Rappaport , A. Vanderburg , T. Jacobs , D. LaCourse , J. Jenkins , A. Kraus , A. Rizzuto , D. W. Latham , A. Bieryla , M. Lazarevic , A. Schmitt

KIC 8462852 is a star in the Kepler field that exhibits almost unique behaviour. The deep, irregular and aperiodic dips in its light curve have been interpreted as the breakup of a large exocomet on a highly eccentric orbit whose…

地球与行星天体物理 · 物理学 2023-09-29 Steven D. Young , Mark C. Wyatt

This paper shows how the dips and secular dimming in the KIC8462852 light curve can originate in circumstellar material distributed around a single elliptical orbit (e.g., exocomets). The expected thermal emission and wavelength dependent…

地球与行星天体物理 · 物理学 2018-06-19 M. C. Wyatt , R. van Lieshout , G. M. Kennedy , T. S. Boyajian

We present millimetre (SMA) and sub-millimetre (SCUBA-2) continuum observations of the peculiar star KIC 8462852 which displayed several deep and aperiodic dips in brightness during the Kepler mission. Our observations are approximately…

Apart from thousands of `regular' exoplanet candidates, Kepler satellite has discovered a few stars exhibiting peculiar eclipse-like events. They are most probably caused by disintegrating bodies transiting in front of the star. However,…

地球与行星天体物理 · 物理学 2017-04-12 L. Neslusan , J. Budaj

Observations of the main sequence F3 V star KIC 8462852 (also known as Boyajian's star) revealed extreme aperiodic dips in flux up to 20% during the four years of the Kepler mission. Smaller dips (< 2%) were also observed with ground-based…

太阳与恒星天体物理 · 物理学 2018-08-06 Gary Sacco , Linh Ngo , Julien Modolo

KIC 8462852 stood out among more than 100,000 stars in the Kepler catalogue because of the strange features of its light curve: a wide, asymmetric dimming taking up to 15 per cent of the light at D793 and a period of multiple, narrow…

地球与行星天体物理 · 物理学 2017-09-29 Fernando J. Ballesteros , Pablo Arnalte-Mur , Alberto Fernandez-Soto , Vicent J. Martinez

This paper discusses an algorithm for detecting single transits in photometric time-series data. Specifically, we aim to identify asymmetric transits with ingress that is more rapid than egress, as expected for cometary bodies with a…

地球与行星天体物理 · 物理学 2018-11-28 Grant M. Kennedy , Greg Hope , Simon T. Hodgkin , Mark C. Wyatt

KIC 8462852 is a superficially ordinary main sequence F star for which Kepler detected an unusual series of brief dimming events. We obtain accurate relative photometry of KIC 8462852 from the Kepler full frame images, finding that the…

太阳与恒星天体物理 · 物理学 2016-10-26 Benjamin T. Montet , Joshua D. Simon

Violent variation of transit depths and an ingress-egress asymmetry of the transit light curve discovered in KIC 12557548 have been interpreted as evidences of a catastrophic evaporation of atmosphere with dust (M_p gtrsim 1 M_oplus/Gyr)…

地球与行星天体物理 · 物理学 2013-10-29 Hajime Kawahara , Teruyuki Hirano , Kenji Kurosaki , Yuichi Ito , Masahiro Ikoma

The Kepler-field star KIC 8462852, an otherwise apparently ordinary F3 main-sequence star, showed several highly unusual dimming events of variable depth and duration. Adding to the mystery was the discovery that KIC 8462852 faded by 14%…

太阳与恒星天体物理 · 物理学 2017-05-31 Brian D. Metzger , Ken J. Shen , Nicholas C. Stone

We analyzed the warm Spitzer/IRAC data of KIC 8462852. We found no evidence of infrared excess at 3.6 micron and a small excess of 0.43 +/- 0.18 mJy at 4.5 micron, below the 3 sigma threshold necessary to claim a detection. The lack of…

太阳与恒星天体物理 · 物理学 2015-11-26 Massimo Marengo , Alan Hulsebus , Sarah Willis

We present optical polarimetry in the period May-August 2017 of the enigmatic "dipping" star KIC 8462852. During that period three ~1% photometric dips were reported by other observers. We measured the average absolute polarization of the…

太阳与恒星天体物理 · 物理学 2017-11-29 I. A Steele , C. M. Copperwheat , H. E. Jermak , G. M. Kennedy , G. P. Lamb

The Kepler object KIC 12557548 shows irregular eclipsing behaviour with a constant 15.685 hr period, but strongly varying transit depth. In this paper we fit individual eclipses, in addition to fitting binned light curves, to learn more…

地球与行星天体物理 · 物理学 2013-11-25 T. I. M. van Werkhoven , M. Brogi , I. A. G. Snellen , C. U. Keller

We report the detection of a single transit-like signal in the Kepler data of the slightly evolved F star KIC4918810. The transit duration is ~45 hours, and while the orbital period ($P\sim10$ years) is not well constrained, it is one of…

Context. The Kepler object KIC 12557548 b is peculiar. It exhibits transit-like features every 15.7 hours that vary in depth between 0.2% and 1.2%. Rappaport et al. (2012) explain the observations in terms of a disintegrating, rocky planet…

地球与行星天体物理 · 物理学 2012-08-17 M. Brogi , C. U. Keller , M. de Juan Ovelar , M. A. Kenworthy , R. J. de Kok , M. Min , I. A. G. Snellen

We present the discovery of KIC 9632895b, a 6.2 Earth-radius planet in a low-eccentricity, 240.5-day orbit about an eclipsing binary. The binary itself consists of a 0.93 and 0.194 solar mass pair of stars with an orbital period of 27.3…

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