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most citedThe size, shape, density and ring of the dwarf planet Haumea from a stellar occultation

258 citations · 662 across the 35 of their papers we have counts for

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Showing 2019Show all

10 papers · 1 filter

astro-ph.SR2019★ 14 cited

Photometric rotation periods for 107 M dwarfs from the APACHE survey

P. Giacobbe, M. Benedetto, M. Damasso +13

We present rotation period measurements for 107 M dwarfs in the mass range observed within the context of the APACHE photometric survey. We measure rotation per…

astro-ph.EP2019

A Case Study of the May 30th, 2017 Italian Fireball

A. Carbognani, D. Barghini, D. Gardiol +25

On May 30th, 2017 at about 21h 09m 17s UTC a green bright fireball crossed the sky of north-eastern Italy. The fireball path was observed from some all-sky cameras starting from a…

astro-ph.EP2019★ 6 cited

A possible YORP effect on C and S Main Belt Asteroids

A. Carbognani

A rotating frequency analysis in a previous paper, showed that two samples of C and S-type asteroids belonging to the Main Belt, but not to any families, present two different valu…

astro-ph.EP2019

Physical characterization of NEA Large Super-Fast Rotator (436724) 2011 UW158

A. Carbognani, B. L. Gary, J. Oey +2

Asteroids of size larger than 0.15 km generally do not have periods smaller than 2.2 hours, a limit known as cohesionless spin barrier. This barrier can be explained by the cohesio…

astro-ph.EP2019

The B-V and V-R Color Indices on the Surface of NEA (214088) 2004 JN13

A. Carbognani

This paper presents the results of photometric observations with standard broad-band Bessel filters B, V, and R on near-Earth asteroid (214088) 2004 JN13. The analysis shows that t…

astro-ph.EP2019★ 5 cited

Statistical analysis of C and S Main Belt Asteroids

A. Carbognani

In this paper we compare the observable properties of 962 numbered MBAs (Main Belt Asteroids) of Tholen/SMASSII C and S class, with diameter in the range 1-500 km, not belonging to…