astrophysics, chemically peculiar stars (CP stars) are stars with distinctly unusual metal abundances, at least in their surface layers. Chemically peculiar stars...
12 KB (1,494 words) - 03:18, 18 November 2024
(abbreviated 20 Tau), is a star in the constellation of Taurus. It is a blue giant of spectral type B8 III, a chemically peculiar star, and the prototype of...
17 KB (1,677 words) - 19:22, 22 October 2024
An Am star or metallic-line star is a type of chemically peculiar star of spectral type A whose spectrum has strong and often variable absorption lines...
7 KB (776 words) - 13:19, 17 July 2024
A mercury-manganese star (also HgMn star) is a type of chemically peculiar star with a prominent spectral line at 398.4 nm, due to absorption from ionized...
5 KB (369 words) - 17:42, 17 November 2024
later revised to A1 IV. It is considered to be a mild Am star, a type of chemically peculiar star with unusually strong lines of certain metallic elements...
15 KB (1,364 words) - 03:31, 15 November 2024
Beta Tauri (redirect from Nath (star))
rarely used. It is a chemically peculiar B7 giant star, 134 light years away from the Sun with an apparent magnitude of 1.65. This star has two Bayer designations:...
16 KB (1,516 words) - 19:22, 19 November 2024
through other means. S-type star, similar, but not as extreme Technetium star, another type of chemically peculiar star Marc Aaronson, American astronomer...
24 KB (2,252 words) - 09:34, 21 October 2024
Alpha Doradus (category Bright Star Catalogue objects)
α Doradus A, is a chemically peculiar star whose atmosphere displays an abnormally high abundance of silicon, making this an Si star. Alpha Doradus has...
8 KB (449 words) - 12:38, 14 May 2023
Gamma Arietis (redirect from Mesarthim (star))
the star rotates. Its brightness varies by 0.04 magnitudes with a period of 2.61 days. It is also an Ap star, a type of chemically peculiar star with...
18 KB (1,442 words) - 07:37, 26 October 2024
A Lambda Boötis star is a type of chemically peculiar star which has an unusually low abundance of iron peak elements in its surface layers. One possible...
2 KB (192 words) - 13:04, 30 July 2023
metal-poor stars, usually referred to as CEMP stars, are a class of chemically peculiar star. CEMP stars have [C/Fe] > +1, which means compared to the Sun these...
2 KB (284 words) - 17:27, 20 February 2024
type of chemically peculiar star with an over-abundance of certain metals in its spectrum. HD 222925 has been referred to as the 'gold standard star' by the...
9 KB (668 words) - 00:24, 18 July 2024
Alioth (redirect from Alioth (star))
701. Sokolov, N. A. (March 2008), "Radial velocity study of the chemically peculiar star ɛ Ursae Majoris", Monthly Notices of the Royal Astronomical Society:...
15 KB (1,332 words) - 03:42, 15 November 2024
abundances of certain metals. A catalogue of chemically peculiar stars gives the type F3 Ho, indicating an Ap star with an approximate spectral class of F3...
22 KB (2,313 words) - 02:55, 9 September 2024
NGC 6633 (category Star cluster stubs)
brightest star is of mag 7.6. Its age has been estimated at 660 million years. The cluster contains at least one chemically peculiar star - NGC 6633...
3 KB (309 words) - 01:02, 16 June 2024
a chemically peculiar star, HR 7775, having extraordinary enhancements of the element gold in its atmosphere. A twenty-year study of the B6III star 3...
12 KB (1,127 words) - 01:14, 2 November 2024
2 Cassiopeiae (category Bright Star Catalogue objects)
constellation Cassiopeia, about 2,800 light years away. It is a chemically peculiar Am star. 2 Cassiopeiae has been described as an A4 type bright giant...
8 KB (717 words) - 22:47, 16 October 2024
Nu Draconis (redirect from Kuma (star))
orbital motion can be observed. 𝜈1 Draconis is an Am star, a slowly rotating chemically peculiar star with abnormally strong metallic absorption lines in...
12 KB (908 words) - 19:58, 18 October 2024
Vega (redirect from Vega (star))
detection of a magnetic field on a spectral class A star that is not an Ap chemically peculiar star. The average line of sight component of this field...
96 KB (10,142 words) - 03:14, 19 November 2024
V2052 Ophiuchi (category Chemically peculiar stars)
from the star's center, and there are helium spots on the surface near the magnetic poles. V2052 Ophiuchi is a type of chemically peculiar star known as...
11 KB (990 words) - 08:36, 18 August 2023
HD 175640 (category Bright Star Catalogue objects)
−26 km/s. This is classified as a mercury-manganese star, which is a late B-type chemically peculiar star of type CP3. A distinctive feature of this class...
8 KB (668 words) - 02:05, 14 November 2024
Alpheratz (redirect from Alpheratz (star))
identified as part of the group of mercury-manganese stars, a class of chemically peculiar stars which have an excess of elements such as mercury, manganese...
29 KB (2,527 words) - 16:40, 26 October 2024
all naturally occurring chemical elements heavier than lithium. Stellar mass loss or supernova explosions return chemically enriched material to the...
148 KB (16,434 words) - 01:14, 22 November 2024
; Malaroda, S. (2000). "A spectroscopic study of the magnetic chemically peculiar star nu Fornacis". Astronomy and Astrophysics. 359: 635–638. Bibcode:2000A&A...
35 KB (4,067 words) - 20:07, 24 August 2024
Ap and Bp stars (redirect from Peculiar A-type star)
Ap and Bp stars are chemically peculiar stars (hence the "p") of spectral types A and B which show overabundances of some metals, such as strontium, chromium...
7 KB (934 words) - 03:41, 7 August 2024
B0–B3 exhibit unusually strong lines of non-ionized helium. These chemically peculiar stars are termed helium-strong stars. These often have strong magnetic...
12 KB (1,369 words) - 11:26, 21 July 2024
HD 28843 (category Objects with variable star designations)
Robert Davis reported that the star has an overabundance of silicon. It is classified as a chemically peculiar star. Henning Jorgensen et al. reported...
12 KB (1,016 words) - 03:28, 23 August 2024
Beta Hydrae (category Bright Star Catalogue objects)
magnitude. It is a magnetic chemically-peculiar star with an average quadratic field strength of (−206±68)×10−4 T. The star is around 178 million years...
13 KB (957 words) - 14:48, 17 July 2024
magnitudes over a period of approximately 1.5 days. Chi Serpentis is a chemically peculiar star. The two stars in Serpens Caput that form part of the Snake's body...
119 KB (11,804 words) - 17:42, 6 November 2024
13 Andromedae (category Bright Star Catalogue objects)
satellite data, and it received its variable star designation in 1999. This is a magnetic chemically peculiar star that has been assigned stellar classifications...
8 KB (653 words) - 22:13, 5 November 2024