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Longer titles found: Red giant (disambiguation) (view), Red giant flying squirrel (view), Red Giant Movies (view), Red Giant Entertainment (view), Red Giant (horse) (view)

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bipolar structure, made up of gas and dust, reflecting light of the central red giant star HR 3126. This is rarely seen because the end-of-life phase of this

40 certain-member stars, two of which have magnitudes 10.5, and a 10.8 red giant, which is the brightest within the cluster. A bright known foreground

cluster in the Milky Way. Abundance measurements of cluster members on the red giant branch show that most are first-generation stars. That is, they did not

2 km/s and thus is a probable runaway star. This is an aging star on the red giant branch with a stellar classification of K4.5IIIa. With the supply of hydrogen

increasingly focused on the long period variables as only AGB and possibly red giant tip stars. The recently classified OSARGs are by far the most numerous

November 28, 1837, by the astronomer John Herschel. Based on the tip of the red-giant branch distance indicator, it lies at a distance of approximately 60 million

Seattle radio station KISW along with an interview with the band. The song "Red Giant" was released on Alice in Chains' official YouTube channel on August 23

measurements gives an estimate of 75 million light years, whereas the tip of the red-giant branch approach yields a distance of 73.4 million light years. It is receding

kpc. Andromeda XXI appears as a spatial overdensity of stars. It has red giant branches at the distance of M31/M33, and follows metal-poor, [Fe/H]=-1

Melbourne continued studies in 1959. Due to the large color spread of its red giant branch (RGB) sequence, akin to that in Omega Centauri, it became the object

velocity of +48 km/s. This is an evolved giant star currently on the red giant branch with a stellar classification of K0 III. The star has 1.35 times

to Gaia magnitude 19. Analysis of 2MASS data for those stars shows a red giant branch and a pronounced red clump that allows the absolute magnitude of

Distance estimates range from 5.39 Mpc to 18.30 Mpc. The tip of the red-giant branch method yields a distance of 11.6 Mpc, while the Tully–Fisher relation

comes to within 124 light-years. This is a K-type subgiant star on the red giant branch track with a stellar classification of K0 IV. It has 1.5 times

to Gaia magnitude 19. Analysis of 2MASS data for those stars shows a red giant branch and a pronounced red clump that allows the absolute magnitude of

from Earth and lies out of the Local Group, determined by the tip of the red giant branch method. The outskirts of the galaxy are harbouring older (reddish)

after a helium flash and ejection of their atmospheres at the tip of the red giant branch. The star contains 10,000 times more zirconium than the Sun; it

Distance estimates range from 5.39 Mpc to 18.30 Mpc. The tip of the red-giant branch method yields a distance of 11.6 Mpc, while the Tully–Fisher relation

only in 1999, with the derivation of a distance based on the tip of the red-giant branch method. Its distance from the Milky Way of 3.2 ±0.2 Mly (980 ±40

age of 740 million years, this is an aging giant star currently on the red giant branch with a stellar classification of G7 III. This indicates it has

helium in its core, although there is a 25% chance that it is still on the red giant branch (RGB) and fusing hydrogen in a shell around an insert core. As

hundred years ago, for example when the red giant reached its critical size. It spiralled towards the red giant but stopped before it merged with the core

velocity of −3.6 km/s. This is an evolved giant star currently on the red giant branch with a stellar classification of K1 III/IV. The luminosity class

classification of G8 IV, indicating that it is a subgiant evolving towards the red giant branch after being an F-type main-sequence star for 1.7 billion years

giant star with a stellar classification of K4 III, currently on the red giant branch. It is around 5.2 billion years old with 1.27 times the mass of

not contain a black hole, but is a mass-transfer binary containing a red giant and a subgiant star that has been stripped of much of its mass. Stellar

giant star with a stellar classification of K5-III, currently on the red giant branch. It has 1.2 times the mass of the Sun and, after consuming the

intermediate spiral galaxy in the constellation Lupus. Based on the tip of the red-giant branch distance indicator, it is located at a distance of about 40 million

and other sources rejecting its membership. However, recent tip of the red-giant branch (TRGB) measurements indicate that NGC 1672 is located at the same

classification of K3 III. Gaia DR3 stellar evolution models place it on the red giant branch. It has a mass comparable to the Sun but due to its evolved state

stellar classification of K0.5 III. It is most likely (78% chance) on the red giant branch and is around 1.55 billion years old. As such, it has an estimated

stellar classification of K2.5 IIIb Fe-1:, most likely (98% chance) on the red giant branch. The suffix notation indicates an underabundance of iron in the

HD 51799 is a class M1III (red giant) star in the constellation Puppis. Its apparent magnitude is 4.95 and it is approximately 860 light years away based

the size of their hydrogen envelope they are found very close to the red giant branch. The two stars are assumed to have the same age, which would be

Earth. With a spectral classification M5IIIa, Tau4 Serpentis is a cool red giant star. The spectrum varies, and some sources classify it between M4IIIe

with a stellar classification of K0 III. It is presently ascending the red-giant branch, having exhausted the supply of hydrogen at its core. The star

classification of G8 IIIa. It is uncertain whether this star is on the red giant branch or the horizontal branch; Reffert et al. (2015) give 57% odd that

on the horizontal branch, fusing helium in its core, but may be on the red giant branch fusing hydrogen in a shell around an insert helium core. It has

−19 km/s. This is an aging giant star, most likely (94% chance) on the red giant branch, with a stellar classification of K4III. It is a suspected variable

carbon is a reflection of internal processes while the star is on the red giant branch, accompanied by deep mixing. In 2000, Böhm-Vitense and collaborators

5II, indicating a bright giant. It is considered likely to be on the red giant branch of stars fusing hydrogen around an inert helium core. Its limb-darkened

(as of 2013). This is an evolved K-type giant star, currently on the red-giant branch, with a stellar classification of K4 III and an estimated age of

stellar classification of K1 III, currently (97% probability) on the red giant branch. It has an estimated 1.36 times the mass of the Sun and has expanded

line. No oxygen or nitrogen has been detected. The star is a K-class red giant. The star was discovered by a team led by Australian National University

R Ursae Minoris is a star in the constellation Ursa Minor. A red giant of spectral type M7IIIe, it is a semiregular variable ranging from magnitude 8

000,000–34,000,000 light-years (5.0–10.3 megaparsecs). The tip of the red-giant branch technique gives a distance of 28,930,000 ± 950,000 light-years

elongated branch is the red giant branch. Some of the stars in the diagram, including those extending outward from the red giant branch toward the upper

star is on the horizontal branch and a 43% chance it is still on the red-giant branch. If it is on the former, the star is estimated to have 1.09 times

simplified statistical analysis suggests that ο Virginis is likely to be a red giant branch star fusing hydrogen in a shell around an inert helium core, but

years, the primary, component A, is a first ascent giant star on the red giant branch with a stellar classification of G8 III, which means it is generating

classification of G8 III, but has most likely not yet made multiple ascents up the red giant branch. It has 3.11 times the mass of the Sun and has expanded to 14 times

represent the final stage before a planetary nebula. During this stage, the red giant star begins to slowly expel its outermost layers of material. A protoplanetary

unusual given the high metallicity of this cluster. Examination of the red giant branch section of the color-magnitude diagram suggests that there are

around half the Sun's. They are thought to have shed mass during the red-giant branch phase, and were once stars at around 0.8 solar masses. In contemporary

is an ageing star, thought to be well on its way transitioning from a red giant to a planetary nebula. A shell of material has been detected at a distance

features visible are a main sequence, and a main sequence turn off, and a red giant branch. It has an unusual enhancement of r-process elements, meaning that

indicating it has ceased hydrogen core fusion and is now evolving toward the red giant branch (RGB). However, Mishenina et al. (2006) said that HD 117566 is

to interstellar dust. This is an orange-hued K-type giant star on the red giant branch, with a stellar classification of K2 III. It has an estimated 1

S Microscopii is a star in the constellation Microscopium. It is a red giant star of spectral type M3e-M5.5 that is also a Mira variable, with an apparent

that has exhausted the supply of hydrogen at its core and is now on the red-giant branch. The 'Ca-1' portion of the classification indicates that it shows

has a stellar classification of G8- IIIa and currently resides on the red giant branch. It has about 390% of the Sun's mass. The star is much younger

et al. (March 2008), "Rotation and Macroturbulence in Metal-Poor Field Red Giant and Red Horizontal Branch Stars", The Astronomical Journal, 135 (3): 892–906

However, S. Reffert and associates in 2015 instead placed it on the red-giant branch. A 2018 study by S. Stock and associates used Bayesian estimates

stellar classification of G8III. It is cooling and expanding along the red giant branch, having evolved off the main sequence after exhausting its core

has a stellar classification of G8- IIIa and currently resides on the red giant branch. It has about 390% of the Sun's mass. The star is much younger

difference of around two billion years. Spectroscopic analysis of the red giant branch member stars suggests there are actually three different populations

stellar classification of G8III. It is cooling and expanding along the red giant branch, having evolved off the main sequence after exhausting its core

velocity of 2.3 km/s. This is an evolved giant star that is currently on the red giant branch, fusing a hydrogen shell around a helium core. HD 222060 a stellar

R Microscopii is a star in the constellation Microscopium. It is a red giant star of spectral type M4e that is also a Mira variable, with an apparent

of K2/3 III — intermediate between a K2 and 3 giant star. It is on the red giant branch, meaning it has exhausted its core hydrogen and is now fusing hydrogen

helium in its core, with just a 13% likelihood that it is still on the red giant branch. The star has 2.51 times the mass of the Sun and has expanded to

probability that it is currently on the horizontal branch, rather than the red giant branch. As such, it is a red clump giant with an estimated 2.43 times

suggests it is an evolved giant star, as stellar models place it on the red giant branch. At present it has 1.6 times the mass of the Sun and at an age

Sketches". IGN. Retrieved 19 June 2015. "Red Giant | NEW Red Giant Film Starring David Hewlett!". Red Giant. 8 November 2017. Retrieved 1 February 2018

Color Description Date of issue Obverse Reverse Obverse Reverse 5 Dalasis Red Giant kingfisher; girl Cattle 2006 10 Dalasis Green Sacred ibis; boy Central

suggests it is an evolved giant star, as stellar models place it on the red giant branch. At present it has 1.6 times the mass of the Sun and at an age

Actress Eliminated Green Giant อาจจะเป็นคนนี้ Undisclosed Advanced to Semi-Final Red Giant Special Song: บัลลังก์เมฆ (Covered by Maneenuch Smerasut [th])

asteroseismologic measurements,enough for it to cool and expand onto the red giant branch; it is now fusing a hydrogen shell around an inert helium core

III, indicating that it is ageing M-type star that is probably on the red giant branch. As a result, it has expanded to 117 times the Sun's girth. At

This object is an aging giant star, most likely (94% chance) on the red giant branch, with a stellar classification of K2III. Having exhausted the hydrogen

hydrogen at its core and left the main sequence. It is currently on the red giant branch, fusing hydrogen in a shell around its helium core. With an expanded

photosphere at an effective temperature of about 4,739 K. It is probably on the red giant branch, which indicates it is generating energy through hydrogen fusion

Warlord miniatures cast by Alternative Armies, and a magazine called Red Giant. The game went out of print 18 months after first publication. Some supplements

cooled and expanded to 53 times the Sun's radius. It most likely on the red giant branch, rather than the asymptotic giant branch, and shows no signs of

titled The Irish Hungarian Guide to the Domestic Arts, was published by Red Giant Books in 2012. She writes the blog "The Erin O'Brien Owner's Manual for

that the object is an ageing K-type giant. Models show it to be on the red giant branch, a stage of stellar evolution where the star is fusing hydrogen

photosphere at an effective temperature of about 4,739 K. It is probably on the red giant branch, which indicates it is generating energy through hydrogen fusion

Warlord miniatures cast by Alternative Armies, and a magazine called Red Giant. The game went out of print 18 months after first publication. Some supplements

intermediate between a G6 and G8 giant star that is currently on the red giant branch. It has 3 times the mass of the Sun but has expanded to 11.7 times

SpaceDaily. 11 January 2015. "Curious spiral spotted by ALMA around red giant star R Sculptoris (data visualisation)". Image Archive. ESO. Retrieved

creators. The company’s product lines include the 3D software Cinema 4D, the Red Giant tools for editing, motion design and filmmaking, Redshift renderer and

giant, meaning it is fusing helium in its core after passing through the red giant branch. The star is 3.2 billion years old with 1.38 times the mass of

IV, indicating that it is an evolved A-type star heading towards the red giant branch. Zorec and Royer (2012) model it as a dwarf star that has just

Punainen jättiläinen ("Red giant") is a Finnish small publisher of Japanese manga and Korean manhwa. It was founded in April 2005 by its CEO, Antti Grönlund

93 L☉. Evolutionary models show that G Scorpii has probably left the red giant branch and is now fusing helium in its core. This makes it a red clump

Label Footnotes 1994 Yatra Rudresh Mahanthappa Red Giant 2002 Black Water Rudresh Mahanthappa Red Giant 2004 Mother Tongue Rudresh Mahanthappa Pi 2006

indicating that it is an evolved giant star. It is currently on the red giant branch, fusing a hydrogen shell around an inert helium core. It has 2

recently experienced the first dredge-up and has begun to ascend the red giant branch although it still has a hot corona and is classified as a subgiant

so-called blue loop phase of its evolution, having already passed through the red-giant branch after exhausting the hydrogen in its core. Canopus is a source

evolved, K-type giant stars, most likely on their first ascent along the red giant branch. The primary, component A, has a stellar classification of K4 III

(4.0 ± 0.2 Mpc). However, NGC 5102 is close enough that the tip of the red giant branch (TRGB) method may be used to estimate its distance. The estimated

.323L..49P Piau, L.; et al. (February 2011), "Surface convection and red-giant radius measurements", Astronomy and Astrophysics, 526: A100, arXiv:1010

ceased but shell burning has not yet started, before ascending towards the red giant branch. Photometric and spectroscopic observations have allowed the direct

clump zone of the HR diagram, which means it has already ascended the red giant branch and is now generating energy by core helium fusion surrounded by

scheduled to be released later in 2010. Their third studio album, titled Red Giant, was released on August 30, 2011. It featured Candlebox singer Kevin Martin

each other in an eccentric orbit. The visible component is an evolved red giant branch (RGB) star with a stellar classification of G9-K0 IIIa, a spectral

1984) Alive in New York (Muse, 1986) Red Giant (SteepleChase, 1988) Red Snapper (SteepleChase, 1988) Red Giant (SteepleChase, 1988) No Turn on Red (Denon

indicating that it is a F-type subgiant that is evolving towards the red giant branch. On the other hand, Nancy Houk and Carrie Swift (1999) found a

IV, indicating that it is a B-type star that is evolving towards the red giant branch. Houk and Cowley (1975) gave a slightly more evolved class of B8/9

be 7.0±0.3 Mly (2.15±0.10 Mpc). At about the same time, the tip of the red giant branch (TRGB) method was used to produce an estimate of 5.9±0.4 Mly (1