activity
20162020
most citedOort spike comets with large perihelion distances

53 citations · 86 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph.EP202018 cited

The Catalogue of Cometary Orbits and their Dynamical Evolution

Małgorzata Królikowska, Piotr A. Dybczyński

The new cometary catalogue containing data for almost 300 long-period comets that were discovered before 2018 is announced (the CODE catalogue). This is the first catalogue contain…

astro-ph.EP20195 cited

First stars that could significantly perturb comet motion are finally found

Rita Wysoczańska, Piotr A. Dybczyński, Małgorzata Królikowska

Since 1950 when Oort published his paper on the structure of the cloud of comets it is believed that stars passing near this hypothetical cometary reservoir play an important role…

astro-ph.EP2019

Kruger 60 as a home system for 2I/Borisov -- a case study

Piotr A. Dybczyński, Małgorzata Królikowska, Rita Wysoczańska

For the second discovered interstellar comet 2I/Borisov we searched for a candidate for its home system. We will never be sure which star or stellar system does this comet come fro…

astro-ph.EP201910 cited

Discovery statistics and the 1/a-distribution of long-period comets detected over the 1801-2017 period

Małgorzata Królikowska, Piotr A. Dybczyński

For the last two decades we have been observing a huge increase in discoveries of long-period comets (LPCs), especially those with large-perihelion distances. We collected data for…

astro-ph.EP2018

Note on the dynamical evolution of C/2017 K2 PANSTARRS

Małgorzata Królikowska, Piotr A. Dybczyński

(Abreviated) Comet C/2017 K2 PANSTARRS drew attention to its activity already at a time of its discovery in May 2017 when it was about 16 au from the Sun. This Oort spike comet wil…

astro-ph.EP201753 cited

Oort spike comets with large perihelion distances

Małgorzata Królikowska, Piotr A. Dybczyński

The complete sample of large-perihelion nearly-parabolic comets discovered during the period 1901-2010 is studied starting from their orbit determination. Next, an orbital evolutio…