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Longer titles found: Metallicity distribution function (view)

searching for Metallicity 19 found (3973 total)

NGC 4429 (413 words) [view diff] no match in snippet view article find links to article

NGC 4429 is a lenticular galaxy located about 55 million light-years away in the constellation of Virgo. NGC 4429 is tilted at an inclination of about

NGC 4478 (506 words) [view diff] no match in snippet view article find links to article

NGC 4478 is an elliptical galaxy located about 50 million light-years away in the constellation Virgo. NGC 4478 was discovered by astronomer William Herschel

NGC 4458 (646 words) [view diff] no match in snippet view article find links to article

NGC 4458 is an elliptical galaxy located about 54 million light-years away in the constellation of Virgo. It was discovered by astronomer William Herschel

Names for sets of chemical elements (528 words) [view diff] no match in snippet view article find links to article

There are currently 118 known chemical elements with a wide range of physical and chemical properties. Amongst this diversity, scientists have found it

Hercules (dwarf galaxy) (915 words) [view diff] exact match in snippet view article

consists mainly of old stars formed more than 12 billion years ago. The metallicity of these old stars is also very low at [Fe/H] ≈ −2.58 ± 0.51, which means

LAMOST 1 (136 words) [view diff] exact match in snippet view article find links to article

light years distant in the Milky Way. The stars have similar age and metallicity. The stars were discovered in spectra from the Large Sky Area Multi-Object

Smith's Cloud (698 words) [view diff] exact match in snippet view article find links to article

hypothesis; these measurements show that the Smith Cloud has an average metallicity of one half of the solar value, indicating that its gas originates in

Palomar 14 (358 words) [view diff] exact match in snippet view article find links to article

about 3–4 billion years younger than a typical galactic cluster. The metallicity of the cluster is [Fe/H] = −1.50, indicating a lower abundance of elements

Leo V (dwarf galaxy) (435 words) [view diff] exact match in snippet view article

consists mainly of old stars formed more than 12 billion years ago. The metallicity of these stars is also very low at [Fe/H] ≈ −2.0 ± 0.2, which means that

Y Sagittarii (469 words) [view diff] exact match in snippet view article find links to article

the Sun. The star's metal content is similar to Sun, with an index of metallicity [Fe / H] = +0.05. For other metals tested, it shows some overabundance

List of planet types (547 words) [view diff] exact match in snippet view article find links to article

deuterium (currently calculated to be 13 Jupiter masses for objects of solar metallicity) that orbit stars, brown dwarfs or stellar remnants and that have a mass

Leo IV (dwarf galaxy) (756 words) [view diff] exact match in snippet view article

consists mainly of old stars formed more than 12 billion years ago. The metallicity of these old stars is also very low at [Fe/H] ≈ −2.58 ± 0.75, which means

Canes Venatici II (659 words) [view diff] exact match in snippet view article find links to article

consists mainly of old stars formed more than 12 billion years ago. The metallicity of these old stars is also very low at [Fe/H] ≈ −2.19±0.58, which means

Canes Venatici I (821 words) [view diff] exact match in snippet view article find links to article

consists mainly of old stars formed more than 10 billion years ago. The metallicity of these old stars is also very low at [Fe/H] ≈ −2.08 ± 0.02, which means

HAT-P-12b (548 words) [view diff] exact match in snippet view article find links to article

core mass of 11.3+2.6 −2.1 M🜨 and is moderately irradiated by its low-metallicity host star. Therefore, HAT-P-12b is most likely an H/He-dominated planet

Ursa Major II Dwarf (601 words) [view diff] exact match in snippet view article find links to article

consists mainly of old stars formed at least 10 billion years ago. The metallicity of these old stars is also very low at [Fe/H] ≈ −2.44 ± 0.06, which means

Ursa Major II Dwarf (601 words) [view diff] exact match in snippet view article find links to article

consists mainly of old stars formed at least 10 billion years ago. The metallicity of these old stars is also very low at [Fe/H] ≈ −2.44 ± 0.06, which means

Strongly correlated material (1,105 words) [view diff] exact match in snippet view article find links to article

properties, such as metal-insulator transitions, heavy fermion behavior, half-metallicity, and spin-charge separation. The essential feature that defines these

IRAS 05280–6910 (593 words) [view diff] exact match in snippet view article find links to article

content, and mass-loss rates of evolved AGB and RSG stars at varying metallicity". Monthly Notices of the Royal Astronomical Society. 465 (1): 403–433