Open AccessCondensations Expelled from the Stars, and Pairs of Stars, Connected with Bright Filaments
Author(s) -
A. L. Gyulbudaghian,
R. A. Mendezz
Publication year - 2021
Publication title -
communications of the byurakan astrophysical observatory
Language(s) - English
Resource type - Journals
ISSN - 2579-2776
DOI - 10.52526/25792776-2021.68.1-90
Subject(s) - stars , physics , astrophysics , infrared , astronomy , star (game theory)
During several surveys of high-quality film-copies of the ESO B, R, ESO/SRC J, and EJ plates, except other young unstable objects (HH objects, star-forming regions, cometary nebulae) were found also two types of other unstable objects. 1. Bright condensations, connected with stars by bright filaments. 2. Pairs of stars, connected with each other by bright filaments. The objects of first type are mostly seen in infrared, on 2MASS K images. Due to their infrared colours, two of condensations and half of all stars can have thick dust discs.