The Pinpoint Comets: 133P/Elst-Pizarro, 249P/LINEAR, 331P/Gibbs, 62412 and 6478 Gault. (arXiv:1907.01096v1 [astro-ph.EP])
<a href="http://arxiv.org/find/astro-ph/1/au:+Ferrin_I/0/1/0/all/0/1">I. Ferr&#xed;n</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Fornari_C/0/1/0/all/0/1">C. Fornari</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Acosta_A/0/1/0/all/0/1">A. Acosta</a>

From two Active Asteroid (AA) known in 1979 we have advanced to 37 members at
the beginning of 2019. More surprisingly, in the first three months of 2019
five new members were added to the list, one of them, 6478 Gault, with a
curious, out of the ordinary tail. This prompted a visual search for similar
objects in images depositories. We have identified five cometary objects that
have the same morphological appearance: A thin long tail coming out of a
star-like nucleus with no gas. The members of this new class (Pinpoint Comet
Group, PCG) are, 133P/Elst-Pizarro, 249P/LINEAR, 331P/Gibbs, 62412 and 6478
Gault. We look for differences and similarities among them. Four of them belong
to the main belt and one to the Jupiter Family of comets. One of them has left
the group but will return soon. Two of them are double. All exhibit densities
well above the Jupiter Family of comets values. This tells us something about
their origin and evolution. In this work we study the secular and rotational
light curves of these objects and their phase and SLC plots. We will
investigate the meaning of these characteristics in terms of their physical
evolution.

From two Active Asteroid (AA) known in 1979 we have advanced to 37 members at
the beginning of 2019. More surprisingly, in the first three months of 2019
five new members were added to the list, one of them, 6478 Gault, with a
curious, out of the ordinary tail. This prompted a visual search for similar
objects in images depositories. We have identified five cometary objects that
have the same morphological appearance: A thin long tail coming out of a
star-like nucleus with no gas. The members of this new class (Pinpoint Comet
Group, PCG) are, 133P/Elst-Pizarro, 249P/LINEAR, 331P/Gibbs, 62412 and 6478
Gault. We look for differences and similarities among them. Four of them belong
to the main belt and one to the Jupiter Family of comets. One of them has left
the group but will return soon. Two of them are double. All exhibit densities
well above the Jupiter Family of comets values. This tells us something about
their origin and evolution. In this work we study the secular and rotational
light curves of these objects and their phase and SLC plots. We will
investigate the meaning of these characteristics in terms of their physical
evolution.

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