eclipsing binary

The two stars form an eclipsing binary system similar to Algol.

A number of visual companions to the eclipsing binary have been observed.

This is a wide eclipsing binary system with an orbital period of 5,329.8 days (14.6 years).

From time to time, the project will observe eclipsing binary stars.

The result is a type of extrinsic variable star system called an eclipsing binary.

He also contributed to the study of eclipsing binaries.

Both A and B have been identified as eclipsing binaries.

The system is also one of the few eclipsing binary symbiotic binaries.

Because the orbital plane is inclined near the line of sight, two form an eclipsing binary system.

The amazing part for me is that they were able to sift through the mountains of data to find this eclipsing binary.

He suggested that Algol is what is now known as an eclipsing binary.

The other two Kids are remarkable eclipsing binaries.

Algol, the prototype eclipsing binary, has been described earlier.

The primary component is an eclipsing binary star in a triple-star grouping.

Some systems exhibit variations in luminosity due to their being eclipsing binaries.

In the era of 8-meter-class telescopes, eclipsing binaries have been found throughout the Local Group.

Algol is the best-known example of an eclipsing binary.

Two of the cluster's star systems are likely eclipsing binaries with periods of 0.6 and 1.03 days.

Polis A is an eclipsing binary, bringing the total of stars in the system to six.

The apparent magnitude of the eclipsing binary varies from 5.65 to 6.05 with a period of 4.4672 days.

We heard a report, for example, from the Eclipsing Binary Working Group.

It is used to monitor eclipsing binary stars and Mira variable stars.

The same phenomenon in eclipsing binaries can make the chromosphere of giant stars visible.

They form an eclipsing binary pair.

It is an eclipsing binary that ranges in magnitude from a minimum of 5.3 to a maximum of 4.8.