These tools will no longer be maintained as of December 31, 2024. Archived website can be found here. PubMed4Hh GitHub repository can be found here. Contact NLM Customer Service if you have questions.
4. White dwarf stars with carbon atmospheres. Dufour P; Liebert J; Fontaine G; Behara N Nature; 2007 Nov; 450(7169):522-4. PubMed ID: 18033290 [TBL] [Abstract][Full Text] [Related]
5. Survival of a brown dwarf after engulfment by a red giant star. Maxted PF; Napiwotzki R; Dobbie PD; Burleigh MR Nature; 2006 Aug; 442(7102):543-5. PubMed ID: 16885979 [TBL] [Abstract][Full Text] [Related]
6. An increase in the Tumino A; Spitaleri C; La Cognata M; Cherubini S; Guardo GL; Gulino M; Hayakawa S; Indelicato I; Lamia L; Petrascu H; Pizzone RG; Puglia SMR; Rapisarda GG; Romano S; Sergi ML; Spartá R; Trache L Nature; 2018 May; 557(7707):687-690. PubMed ID: 29795352 [TBL] [Abstract][Full Text] [Related]
7. Trions in bulk and monolayer materials: Faddeev equations and hyperspherical harmonics. Filikhin I; Kezerashvili RY; Tsiklauri SM; Vlahovic B Nanotechnology; 2018 Mar; 29(12):124002. PubMed ID: 29350620 [TBL] [Abstract][Full Text] [Related]
8. Crystallization of carbon-oxygen mixtures in white dwarf stars. Horowitz CJ; Schneider AS; Berry DK Phys Rev Lett; 2010 Jun; 104(23):231101. PubMed ID: 20867223 [TBL] [Abstract][Full Text] [Related]
9. Measurement of 23Na(α,p)26Mg at Energies Relevant to 26Al Production in Massive Stars. Tomlinson JR; Fallis J; Laird AM; Fox SP; Akers C; Alcorta M; Bentley MA; Christian G; Davids B; Davinson T; Fulton BR; Galinski N; Rojas A; Ruiz C; de Séréville N; Shen M; Shotter AC Phys Rev Lett; 2015 Jul; 115(5):052702. PubMed ID: 26274415 [TBL] [Abstract][Full Text] [Related]
10. Three New Low-Energy Resonances in the ^{22}Ne(p,γ)^{23}Na Reaction. Cavanna F; Depalo R; Aliotta M; Anders M; Bemmerer D; Best A; Boeltzig A; Broggini C; Bruno CG; Caciolli A; Corvisiero P; Davinson T; di Leva A; Elekes Z; Ferraro F; Formicola A; Fülöp Z; Gervino G; Guglielmetti A; Gustavino C; Gyürky G; Imbriani G; Junker M; Menegazzo R; Mossa V; Pantaleo FR; Prati P; Scott DA; Somorjai E; Straniero O; Strieder F; Szücs T; Takács MP; Trezzi D; Phys Rev Lett; 2015 Dec; 115(25):252501. PubMed ID: 26722918 [TBL] [Abstract][Full Text] [Related]
11. (22)Ne(alpha,n)(25)Mg: the key neutron source in massive stars. Jaeger M; Kunz R; Mayer A; Hammer JW; Staudt G; Kratz KL; Pfeiffer B Phys Rev Lett; 2001 Nov; 87(20):202501. PubMed ID: 11690469 [TBL] [Abstract][Full Text] [Related]
13. Discovery of two young brown dwarfs in an eclipsing binary system. Stassun KG; Mathieu RD; Valenti JA Nature; 2006 Mar; 440(7082):311-4. PubMed ID: 16541067 [TBL] [Abstract][Full Text] [Related]
14. Sodium content as a predictor of the advanced evolution of globular cluster stars. Campbell SW; D'Orazi V; Yong D; Constantino TN; Lattanzio JC; Stancliffe RJ; Angelou GC; Wylie-de Boer EC; Grundahl F Nature; 2013 Jun; 498(7453):198-200. PubMed ID: 23719375 [TBL] [Abstract][Full Text] [Related]
15. Improved Direct Measurement of the 64.5 keV Resonance Strength in the ^{17}O(p,α)^{14}N Reaction at LUNA. Bruno CG; Scott DA; Aliotta M; Formicola A; Best A; Boeltzig A; Bemmerer D; Broggini C; Caciolli A; Cavanna F; Ciani GF; Corvisiero P; Davinson T; Depalo R; Di Leva A; Elekes Z; Ferraro F; Fülöp Z; Gervino G; Guglielmetti A; Gustavino C; Gyürky G; Imbriani G; Junker M; Menegazzo R; Mossa V; Pantaleo FR; Piatti D; Prati P; Somorjai E; Straniero O; Strieder F; Szücs T; Takács MP; Trezzi D; Phys Rev Lett; 2016 Sep; 117(14):142502. PubMed ID: 27740778 [TBL] [Abstract][Full Text] [Related]
16. Measurement of the -3 keV resonance in the reaction 13C(α,n)16O of importance in the s-process. La Cognata M; Spitaleri C; Trippella O; Kiss GG; Rogachev GV; Mukhamedzhanov AM; Avila M; Guardo GL; Koshchiy E; Kuchera A; Lamia L; Puglia SM; Romano S; Santiago D; Spartà R Phys Rev Lett; 2012 Dec; 109(23):232701. PubMed ID: 23368189 [TBL] [Abstract][Full Text] [Related]
17. Radial velocity studies of cool stars. Jones HR; Barnes J; Tuomi M; Jenkins JS; Anglada-Escude G Philos Trans A Math Phys Eng Sci; 2014 Apr; 372(2014):20130088. PubMed ID: 24664922 [TBL] [Abstract][Full Text] [Related]
18. 11B and constraints on neutrino oscillations and spectra from neutrino nucleosynthesis. Austin SM; Heger A; Tur C Phys Rev Lett; 2011 Apr; 106(15):152501. PubMed ID: 21568548 [TBL] [Abstract][Full Text] [Related]
19. Using self-organizing maps to identify potential halo white dwarfs. García-Berro E; Torres S; Isern J Neural Netw; 2003; 16(3-4):405-10. PubMed ID: 12672435 [TBL] [Abstract][Full Text] [Related]
20. The formation of stars by gravitational collapse rather than competitive accretion. Krumholz MR; McKee CF; Klein RI Nature; 2005 Nov; 438(7066):332-4. PubMed ID: 16292305 [TBL] [Abstract][Full Text] [Related] [Next] [New Search]