subgiant star

It is a blue subgiant star, seven hundred times more luminous than the Sun.

It is a yellow dwarf or subgiant star of mass 7% greater than our Sun.

In several tens of millions of years it will likely become a subgiant star.

It is the nearest subgiant star to the Sun and one of the oldest stars in the solar neighborhood.

This is a subgiant star, having a stellar classification of A7 IV.

It is a bluish white subgiant star of the spectral type B6IV.

The planet was discovered in a close-orbit around the yellow subgiant star HD 11964.

It is classified as a yellow subgiant star (spectral type G5IV).

HD 175541 is an intermediate-mass subgiant star in the constellation Serpens.

Theta Columbae is a blue subgiant star in the constellation Columba.

Due to its unusually brightness, at least one source suspects that the star may be a highly evolved subgiant star.

There is a binary star system at the center with a B1 dwarf orbiting a B3 subgiant star.

HD 100777 is an orange subgiant star located approximately 172 light years away in the constellation Leo.

HR 8938 is a subgiant star near the north celestial pole in the constellation Cepheus.

HD 11964 is a yellow subgiant star approximately 107 light-years away in the constellation of Cetus.

HD 2039 is a yellow dwarf or yellow subgiant star in the constellation Phoenix.

It has an apparent brightness of +4.13 magnitude and belongs to the spectral class F5IV; a subgiant star.

Back in 1999 the presence of a planetary companion was inferred around Gamma Delphini, an evolved orange subgiant star.

At the age of 2.8 billion years, it has reached an evolutionary stage called a subgiant star, having a stellar classification of G5 IV.

The planet was announced orbiting the yellow subgiant star Pi Mensae in October 2001.

Tau Herculis is a blue subgiant star with stellar classification B5IV.

It is an orange K-type subgiant star, meaning it has nearly completely exhausted its hydrogen supply in its core.

Delta Geminorum is a subgiant star with the stellar classification F0 IV.

The primary component has a stellar classification of A0 IVs, indicating that it is a subgiant star.

It has a stellar classification of B2 IV, which matches a massive B-type subgiant star.