We present a model of the dust environment of Main-Belt Comet P/2010 R2 (La Sagra) from images acquired during the period 2010 October-2011 January. The tails...
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PublicaciónThe Dust Environment of Main-Belt Comet P/2010 R2 (La Sagra)
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PublicaciónThe Dust Environment of Main-Belt Comet P/2012 T1 (PANSTARRS)
The Main-Belt Comet P/2012 T1 (PANSTARRS) has been imaged using the 10.4 m Gran Telescopio Canarias and the 4.2 m William Herschel Telescope at six epochs in...
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PublicaciónThe dust tail of Comet C/1999 T1 McNaught-Hartley
A numerical method to compute cometary dust tail brightnesses has been developed. The method, analogous in many ways to the inverse Monte Carlo method proposed...
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PublicaciónThe Effect of Seeing Variations in Time-Series CCD Inner Coma Photometry of Comets: A New Correction Method
Time series CCD photometry of the inner coma of active comets has been used over the last twenty years to determine the rotation period of their nucleus...
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PublicaciónThe First Post-Kepler Brightness Dips of KIC 8462852
We present a photometric detection of the first brightness dips of the unique variable star KIC 8462852 since the end of the Kepler space mission in 2013 May...
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PublicaciónThe nature of comet-asteroid transition object (3200) Phaethon
Context: The study of asteroids that present sporadic cometary activity is of fundamental importance to address several astronomical problems including the end...
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PublicaciónThe population, magnitudes, and sizes of Jupiter family comets
We analyze the sample of measured nuclear magnitudes of the observed Jupiter family (JF) comets (taken as those with orbital periods P < 20 years and Tisserand...
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PublicaciónThe Rotation Period of C/1995 01 (Hale-Bopp)
C/1995 O1 (Hale-Bopp) was observed in daylight on 16 days between 1997 April 1 and 1997 April 28, five of which had long time sequences (up to 10 hr of data)...
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PublicaciónThe Rotation Period of C/2014 Q2 (Lovejoy)
C/2014 Q2 (Lovejoy) was observed around perihelion (2015 January 30) on 15 nights between 2015 January 21 and February 11 using the TADer 0.3-m astrograph...