Struve 2653 - A binary star, in a telescope with an objective diameter of up to 150 mm, is a very close pair of unequally bright yellow-white stars (6.9 mag, 9.7 mag), which require appropriate magnification for resolution. They are separated by only 2.6".

Burnham 441 - This double star could be observed with a 100 mm telescope. It presents as a color contrast between a golden and blue component. The difference in magnitude is significant, with the golden component reaching 6.2 mag and the blue component only 10.7 mag. It is located at a separation of 5.9".

Struve 2455 - In a 100 mm telescope, the triple star is an attractive pair of one white and two bluish components. The brightest components (7.4 mag and 8.5 mag) are separated by 6.6". Half a degree to the NNE, in the same field of view, there is the double star Struve 2457, consisting of a white 7.5 mag component and a bluish 9 mag component, separated by 10.3".

Struve 2540 - Constellation. In a 100/150 mm instrument, a relatively close pair (5.1") consists of unequally bright white component of magnitude 7.3 and a blue component of magnitude 8.8. The companion of magnitude 12.4 is located 147" away.