irregular variable star

We're almost better off doing nothing at all rather than trying to tickle an irregular variable star."

However, it appears to possess the characteristics of an irregular variable star."

It was observed to be an irregular variable star ranging from 12 to 14 in apparent magnitude.

It is classified as an irregular variable star and its brightness varies from magnitude +5.2 to +5.3.

The irregular variable star Z Sagittae is a member of this cluster.

These blazars, like genuine irregular variable stars, changed in brightness on periods of days or years, but with no pattern.

It is cataloged as an irregular variable star, and it has an oscilation period of 201 days.

Mu Chamaeleontis is an irregular variable star.

RW Aurigae is the prototype of its class of irregular variable stars.

H Centauri is a suspected triple star system, and is a long period irregular variable star.

It has never been observed since, but that does not preclude the possibility of it being a highly irregular variable star or a recurrent nova.

R Coronae Australis is an irregular variable star ranging from magnitudes 9.7 to 13.9.

Many of the brighter blazars were first identified, not as powerful distant galaxies, but as irregular variable stars in our own galaxy.

"In the meantime, I'll also keep watch on this irregular variable star...which is far from being stable in any regard.

U Antliae is a red C-type carbon star and is an irregular variable star.

We've certainly made an outstanding discovery here...an isolated planet orbiting an irregular variable star in the interarm void.

The primary is an irregular variable star; it is a red giant with a minimum magnitude of 4 and a maximum magnitude of 3.

It is located near the open cluster NGC 637, and the bright magnitude +2.2 irregular variable star Gamma Cassiopeiae.

What sort of a life form are we going to encounter that could develop on an extremely isolated planet around an irregular variable star located several hundred parsecs from any other star?"

It was first discovered by Cuno Hoffmeister in 1929, but was originally thought to be an irregular variable star in the Milky Way galaxy and so was given a variable star designation.

It surrounds the irregular variable star AE Aurigae and is located near the emission nebula IC 410, the open clusters M38 and M36, and the naked-eye K-class star Hassaleh.

As depicted in the original Battlestar Galactica series (1978-79), particularly the series episode "Lost Planet of the Gods", Kobol orbits an irregular variable star, and its encompassing system of planets lies immediately adjacent to a "magnetic void".

Kirk had gathered that the Guardians had considerable political power over the people of Mercan because of the Guardian possession of the Mystery of the Ordeal-the ability to predict the flare-ups of the Mercaniad irregular variable star.

On early 20th century and older orthochromatic (blue-sensitive) photographic film, the relative brightnesses of the blue supergiant Rigel and the red supergiant Betelgeuse irregular variable star (at maximum) are reversed compared to what our eyes see since this archaic film is more sensitive to blue light than it is to red light.