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相关论文: Photometric Observations of 107P/Wilson-Harrington

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We analyzed images of comet 49P/Arend-Rigaux on 33 nights between 2012 January and May and obtained R-band lightcurves of the nucleus. Through usual phasing of the data we found a double-peaked lightcurve having a synodic rotation period of…

地球与行星天体物理 · 物理学 2017-10-25 Nora Eisner , Matthew M. Knight , David G. Schleicher

We used the optical and near-infrared imagers located on the Liverpool, the IAC80, and the William Herschel telescopes to monitor 18 M7$-$L9.5 dwarfs with the objective of measuring their rotation periods. We achieved accuracies typically…

太阳与恒星天体物理 · 物理学 2017-09-27 P. A. Miles-Páez , E. Pallé , M. R. Zapatero Osorio

We report on narrowband CN imaging of Comet 103P/Hartley 2 obtained at Lowell Observatory on 39 nights from 2010 July until 2011 January. We observed two features, one generally to the north and the other generally to the south. The CN…

地球与行星天体物理 · 物理学 2015-05-27 Matthew M. Knight , David G. Schleicher

We present highly time resolved circular-polarization and flux spectra of the magnetic white dwarf LP790-29 taken with the VLT UT1 in order to test the hypothesis that LP790-29 is a fast rotator with a period of the order of seconds to…

天体物理学 · 物理学 2009-11-07 Stefan Jordan , Susanne Friedrich

We report on photometry and imaging of Comet 103P/Hartley 2 obtained at Lowell Observatory from 1991 through 2011. We acquired photoelectric photometry on two nights in 1991, four nights in 1997/98, and 13 nights in 2010/11. We observed a…

地球与行星天体物理 · 物理学 2015-06-05 Matthew M. Knight , David G. Schleicher

We first present the multicolor photometry results of the rapidly rotating magnetic star HD 345439 using the Nanshan One-meter Wide-field Telescope. From the photometric observations, we derive a rotational period of 0.7699\pm0.0014 day.…

We present new analyses of the photometric lightcurve of Comet 1P/Halley during its 1985/86 apparition. As part of a world-wide campaign coordinated by the International Halley Watch (IHW), narrowband photometry was obtained with telescopes…

Comet 107P/Wilson-Harrington, cross-listed as asteroid 4015, is one of the original transition objects whose properties do not neatly fit into a cometary or asteroidal origin. Discovered in a period of apparently gas-dominated activity in…

地球与行星天体物理 · 物理学 2023-08-21 Theodore Kareta , Vishnu Reddy

WASP-33b is a retrograde hot Jupiter with a period of 1.2 days orbiting around a rapidly rotating and pulsating A-type star. A previous study found that the transit chord of WASP-33b had changed slightly from 2008 to 2014 based on Doppler…

地球与行星天体物理 · 物理学 2020-03-06 Noriharu Watanabe , Norio Narita , Marshall C. Johnson

We present results from CCD observations of comet 2P/Encke acquired at Steward Observatory's 2.3m Bok Telescope on Kitt Peak obtained in Oct. 2002, when the comet was near aphelion. Rotational lightcurves in B, V and R-filters were acquired…

天体物理学 · 物理学 2009-11-11 S. C. Lowry , P. R. Weissman

We analyse optical and X-ray spectroscopy of the Of?p star HD108, known for its strong dipolar magnetic field and its optical line profile variability with a timescale of $54 \pm 3$ yrs, interpreted as the stellar rotation period. Optical…

太阳与恒星天体物理 · 物理学 2023-03-15 Gregor Rauw , Yaël Nazé , Asif ud-Doula , Coralie Neiner

We report on photometry and imaging of Comet 10P/Tempel 2 obtained at Lowell Observatory from 1983 through 2011. We measured a nucleus rotation period of 8.950 +/- 0.002 hr from 2010 September to 2011 January. This rotation period is longer…

地球与行星天体物理 · 物理学 2015-06-11 Matthew M. Knight , David G. Schleicher , Tony L. Farnham , Edward W. Schwieterman , Samantha R. Christensen

We present the results of an intensive photometric and spectroscopic monitoring campaign of the WN4 Wolf-Rayet (WR) star WR1=HD4004. Our broadband V photometry covering a timespan of 91 days shows variability with a period of…

太阳与恒星天体物理 · 物理学 2015-05-18 André-Nicolas Chené , Nicole St-Louis

We present new lightcurve measurements of Comet 10P/Tempel 2 carried out with Lowell Observatory's Discovery Channel Telescope in early 2013 when the comet was at aphelion. These data represent some of the first science obtained with this…

地球与行星天体物理 · 物理学 2015-06-17 David G. Schleicher , Matthew M. Knight , Stephen E. Levine

We report on our extensive photometry and imaging of Comet 46P/Wirtanen during its 2018/19 apparition and use these data to constrain modeling of Wirtanen's activity. Narrowband photometry was obtained on nine epochs from 2018 October…

地球与行星天体物理 · 物理学 2021-03-26 Matthew M. Knight , David G. Schleicher , Tony L. Farnham

We present photometry of HD 189733 during eight transits of its close-in giant planet, and out-of-transit photometry spanning two years. Using the transit photometry, we determine the stellar and planetary radii and the photometric…

We present 17 nights of ground-based, near-infrared photometry of the variable L/T transition brown dwarf SIMP J013656.5+093347 and an additional 3 nights of ground-based photometry of the radio-active late M-dwarf TVLM 513-46546. Our TVLM…

太阳与恒星天体物理 · 物理学 2016-09-14 Bryce Croll , Philip S. Muirhead , Jack Lichtman , Eunkyu Han , Paul A. Dalba , Jacqueline Radigan

We present Spitzer Space Telescope time-series photometry at 3.6 and 4.5 $\mu$m of 2MASS J11193254$-$1137466AB and WISEA J114724.10$-$204021.3, two planetary-mass, late-type ($\sim$L7) brown dwarf members of the $\sim$10 Myr old TW Hya…

太阳与恒星天体物理 · 物理学 2018-05-23 Adam C. Schneider , Kevin K. Hardegree-Ullman , Michael C. Cushing , J. Davy Kirkpatrick , Evgenya L. Shkolnik

The photometric light curve of PG1302-102 shows periodic variability which makes this object one of the most plausible supermassive black hole binary candidate. Interestingly, the most recent study of its updated optical light curve reports…

高能天体物理现象 · 物理学 2019-01-30 Andjelka B. Kovacevic , Luka C. Popovic , Sasa Simic , Dragana Ilic

By analysing the K2 short-cadence photometry we detect starspot occultation events in the lightcurve of WASP-107, the host star of a warm-Saturn exoplanet. WASP-107 also shows a rotational modulation with a period of 17.5 +/- 1.4 d. Given…

地球与行星天体物理 · 物理学 2017-04-25 T. Močnik , C. Hellier , D. R. Anderson , B. J. M. Clark , J. Southworth
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