activity
20072024
most citedHD 17156b: A Transiting Planet with a 21.2 Day Period and an Eccentric Orbit

98 citations · 595 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.EP2024

Comet 81/P Wild 2: changes in the spin axis orientation during the last five apparitions

V. Oldani, F. Manzini, P. Ochner +8

Comet 81P (Wild 2) is characterized by the presence of a prominent-fan shaped dust emission originating from an active source at high latitude on the nucleus, whose axis is assumed…

astro-ph.EP2021

Radial Distribution of the Dust Comae of Comets 45P/Honda-Mrkos-Pajduusáková and 46P/Wirtanen

C. Lejoly, W. Harris, N. Samarasinha +21

There was an unprecedented opportunity to study the inner dust coma environment, where the dust and gas are not entirely decoupled, of comets 45P/Honda-Mrkos-Pajduusáková (45P/HMP)…

astro-ph.EP2021★ 14 cited

Coma morphology and dust emission pattern of comet C/2020 F3 (NEOWISE)

F. Manzini, V. Oldani, P. Ochner +4

The recent close approach of comet C/2020 F3 (NEOWISE) allowed us to study the morphology of its inner coma. From the measurement of the dust ejection velocityon spiral structures…

astro-ph.EP2021★ 16 cited

Properties of slowly rotating asteroids from the Convex Inversion Thermophysical Model

A. Marciniak, J. Ďurech, V. Alí-Lagoa +73

Results from the TESS mission showed that previous studies strngly underestimated the number of slow rotators, revealing the importance of studying those asteroids. For most slowly…

astro-ph.EP2020★ 18 cited

Interstellar Comet 2I/Borisov exhibits a structure similar to native Solar System comets

F. Manzini, V. Oldani, P. Ochner +2

We processed images taken with the Hubble Space Telescope (HST) to investigate any morphological features in the inner coma suggestive of a peculiar activity on the nucleus of the…

astro-ph.EP2019★ 29 cited

Thermal properties of slowly rotating asteroids: Results from a targeted survey

A. Marciniak, V. Alí-Lagoa, T. G. Müller +51

Context. Earlier work suggests that slowly rotating asteroids should have higher thermal inertias than faster rotators because the heat wave penetrates deeper into the sub-surface.…