red clump in a sentence

• This is a red clump giant star with a stellar classification of K2 IIIb.
• Stars with will also pass through the red clump as they evolve along the subgiant branch.
• It is a red clump giant.
• Kappa Ophiuchi belongs to an evolutionary branch known as the red clump, making it a clump giant.
• The brightest and higher temperature members of the red clump stars are more concentrated toward the center of the cluster.
• It is in the red clump, meaning it is generating energy through the fusion of helium into carbon at its core.
• The readjustment following the flash brings the red giant to the so-called red clump ( RC ) in the Hertzsprung-Russell diagram.
• There is a considerable spread in the properties of red clump stars even within a single population of similar stars such as an open cluster.
• ? Andromedae is believed to be a red clump star which is eccentric, causing it to move rapidly relative to the Sun and its neighboring stars.
• Many of these helium-fusing stars cluster towards the cool end of the horizontal branch as K-type giants and are referred to red clump giants.
• It's difficult to see red clump in a sentence .
• These stars are often observed as a red clump of stars in the colour-magnitude diagram of a cluster, hotter and less luminous than the red giants.
• This occurs in ? Centauri where metal-poor red-giant-branch stars have the same or hotter temperatures as more metal-rich red clump giants.
• For stars only a little more massive than the sun, around, the blue loop is very short and at a luminosity similar to the red clump giants.
• In the 1990s, measurements of both standard red giants as well as red clump stars from the " Hipparcos " satellite measurements were used to calibrate the Cepheid distances.
• "' Psi 1 Lupi "'( ? 1 Lupi ) is an red clump giant star located 205 light years away from the Sun, in the Lupus constellation.
• Presently it is generating energy through the nuclear fusion of helium at its core, which, considering the star's composition, places it along an evolutionary branch termed the red clump.
• Although red clump stars lie consistently to the hot side of the red giant branch that they evolved from, red clump and red-giant-branch stars from different populations can overlap.
• Although red clump stars lie consistently to the hot side of the red giant branch that they evolved from, red clump and red-giant-branch stars from different populations can overlap.
• More recently, this inclined geometry for field stars in the LMC has been confirmed via observations of Cepheids, core helium-burning red clump stars and the tip of the red giant branch.
• Although red clump stars are generally hotter than red-giant-branch stars, the two regions overlap and the status of individual stars can only be assigned with a detailed chemical abundance study.