ε CrA - An eclipsing variable star with a period of 14 hours. Since it is located on the northern edge of the constellation, it can be seen here as well, at least from areas at higher altitudes and without light pollution.

γ CrA - tight binary star, whose equally bright 5th magnitude components orbit each other every 120 years. We can distinguish them with a larger telescope. It is located at a distance of 58 light years.

κ CrA - A remarkable binary star in the rich Milky Way, whose both blue-white companions with magnitudes of 5.9 and 6.6 have a separation of 21.4 arcseconds. Therefore, they can be easily distinguished even in a small telescope.

Brisbane 14 - The double star observed only 12' WSW of the reflection nebula NGC 6726-27, as a nearly equally bright pair of blue-white components with magnitudes 6.6 and 6.8, which can be resolved even with a small telescope. The mutual separation of the components is 12.7".

RX J185635-3754 - Under this obscure designation hides our closest neutron star, which is located at a distance of 200 light-years. With its apparent magnitude of 26mag, it cannot be observed in any case, it was discovered only in 1996 by the Hubble Space Telescope. It is a remnant of a supernova explosion that occurred a million years ago.