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.


BIOMARKERS

Molecular Biopsy of Human Tumors

- a resource for Precision Medicine *

125 related articles for article (PubMed ID: 23403570)

  • 1. Si:P as a laboratory analogue for hydrogen on high magnetic field white dwarf stars.
    Murdin BN; Li J; Pang ML; Bowyer ET; Litvinenko KL; Clowes SK; Engelkamp H; Pidgeon CR; Galbraith I; Abrosimov NV; Riemann H; Pavlov SG; Hübers HW; Murdin PG
    Nat Commun; 2013; 4():1469. PubMed ID: 23403570
    [TBL] [Abstract][Full Text] [Related]  

  • 2. Quadratic Zeeman effect in hydrogen at 2-3 MG magnetic fields.
    Ivanov VV; Mancini RC; Huerta NA; Swanson KJ; Winget DE; Montgomery MH; Golovkin IE; Hariharan HK; Berbel ZS
    Phys Rev E; 2022 Oct; 106(4-2):045206. PubMed ID: 36397480
    [TBL] [Abstract][Full Text] [Related]  

  • 3. Suppression of cooling by strong magnetic fields in white dwarf stars.
    Valyavin G; Shulyak D; Wade GA; Antonyuk K; Zharikov SV; Galazutdinov GA; Plachinda S; Bagnulo S; Machado LF; Alvarez M; Clark DM; Lopez JM; Hiriart D; Han I; Jeon YB; Zurita C; Mujica R; Burlakova T; Szeifert T; Burenkov A
    Nature; 2014 Nov; 515(7525):88-91. PubMed ID: 25327247
    [TBL] [Abstract][Full Text] [Related]  

  • 4. Gigagauss magnetic field measurements using Zeeman broadening of Ne-like transitions in highly charged ions.
    Seely JF
    Rev Sci Instrum; 2021 May; 92(5):053535. PubMed ID: 34243271
    [TBL] [Abstract][Full Text] [Related]  

  • 5. Limits on a gravitational field dependence of the proton-electron mass ratio from H2 in white dwarf stars.
    Bagdonaite J; Salumbides EJ; Preval SP; Barstow MA; Barrow JD; Murphy MT; Ubachs W
    Phys Rev Lett; 2014 Sep; 113(12):123002. PubMed ID: 25279624
    [TBL] [Abstract][Full Text] [Related]  

  • 6. Metal abundances in hot white dwarfs with signatures of a superionized wind.
    Werner K; Rauch T; Kruk JW
    Astron Astrophys; 2018 Jan; 609():. PubMed ID: 32020917
    [TBL] [Abstract][Full Text] [Related]  

  • 7. Spherical, cylindrical and tetrahedral symmetries; hydrogenic states at high magnetic field in Si:P.
    Lewis RA; Bruno-Alfonso A; de Souza GV; Vickers RE; Colla JA; Constable E
    Sci Rep; 2013 Dec; 3():3488. PubMed ID: 24336145
    [TBL] [Abstract][Full Text] [Related]  

  • 8. A highly magnetized and rapidly rotating white dwarf as small as the Moon.
    Caiazzo I; Burdge KB; Fuller J; Heyl J; Kulkarni SR; Prince TA; Richer HB; Schwab J; Andreoni I; Bellm EC; Drake A; Duev DA; Graham MJ; Helou G; Mahabal AA; Masci FJ; Smith R; Soumagnac MT
    Nature; 2021 Jul; 595(7865):39-42. PubMed ID: 34194021
    [TBL] [Abstract][Full Text] [Related]  

  • 9. Magnetically gated accretion in an accreting 'non-magnetic' white dwarf.
    Scaringi S; Maccarone TJ; D'Angelo C; Knigge C; Groot PJ
    Nature; 2017 Dec; 552(7684):210-213. PubMed ID: 29239355
    [TBL] [Abstract][Full Text] [Related]  

  • 10. GW quasiparticle energies of atoms in strong magnetic fields.
    Holzer C; Teale AM; Hampe F; Stopkowicz S; Helgaker T; Klopper W
    J Chem Phys; 2019 Jun; 150(21):214112. PubMed ID: 31176321
    [TBL] [Abstract][Full Text] [Related]  

  • 11. 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]  

  • 12. Formation of high-field magnetic white dwarfs from common envelopes.
    Nordhaus J; Wellons S; Spiegel DS; Metzger BD; Blackman EG
    Proc Natl Acad Sci U S A; 2011 Feb; 108(8):3135-40. PubMed ID: 21300910
    [TBL] [Abstract][Full Text] [Related]  

  • 13. 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]  

  • 14. Physics in strong magnetic fields near neutron stars.
    Harding AK
    Science; 1991 Mar; 251(4997):1033-8. PubMed ID: 17802087
    [TBL] [Abstract][Full Text] [Related]  

  • 15. A fossil origin for the magnetic field in A stars and white dwarfs.
    Braithwaite J; Spruit HC
    Nature; 2004 Oct; 431(7010):819-21. PubMed ID: 15483604
    [TBL] [Abstract][Full Text] [Related]  

  • 16. Infrared absorption by collisional H2-He complexes at temperatures up to 9000 K and frequencies from 0 to 20,000 cm(-1).
    Abel M; Frommhold L; Li X; Hunt KL
    J Chem Phys; 2012 Jan; 136(4):044319. PubMed ID: 22299883
    [TBL] [Abstract][Full Text] [Related]  

  • 17. Low density of neutral hydrogen and helium in the local interstellar medium: Extreme Ultraviolet Explorer photometry of the Lyman continuum of the hot white dwarfs MCT 0501-2858, MCT 0455-2812, HZ 43, and GD 153.
    Vennes S; Dupuis J; Bowyer S; Fontaine G; Wiercigroch A; Jelinsky P; Wesemael F; Malina R
    Astrophys J; 1994 Jan; 421(1 Pt 2):L35-8. PubMed ID: 11539405
    [TBL] [Abstract][Full Text] [Related]  

  • 18. Accreting neutron stars, black holes, and degenerate dwarf stars.
    Pines D
    Science; 1980 Feb; 207(4431):597-606. PubMed ID: 17749313
    [TBL] [Abstract][Full Text] [Related]  

  • 19. Ab Initio molecular dynamics with screened Lorentz forces. II. Efficient propagators and rovibrational spectra in strong magnetic fields.
    Peters LDM; Culpitt T; Monzel L; Tellgren EI; Helgaker T
    J Chem Phys; 2021 Jul; 155(2):024105. PubMed ID: 34266256
    [TBL] [Abstract][Full Text] [Related]  

  • 20. Energy flux determines magnetic field strength of planets and stars.
    Christensen UR; Holzwarth V; Reiners A
    Nature; 2009 Jan; 457(7226):167-9. PubMed ID: 19129842
    [TBL] [Abstract][Full Text] [Related]  

    [Next]    [New Search]
    of 7.