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 *

115 related articles for article (PubMed ID: 11539919)

  • 1. A correlated ab initio study of linear carbon-chain radicals CnH (n = 2-7).
    Woon DE
    Chem Phys Lett; 1995 Sep; 244():45-52. PubMed ID: 11539919
    [TBL] [Abstract][Full Text] [Related]  

  • 2. A correlated ab initio study of the A2 pi <-- X2 sigma+ transition in MgCCH.
    Woon DE
    Chem Phys Lett; 1997 Aug; 274():299-305. PubMed ID: 11541845
    [TBL] [Abstract][Full Text] [Related]  

  • 3. Is interstellar detection of higher members of the linear radicals CnCH and CnN feasible?
    Pauzat F; Ellinger Y; McLean AD
    Astrophys J; 1991 Mar; 369():L13-6. PubMed ID: 11538264
    [TBL] [Abstract][Full Text] [Related]  

  • 4. An ab initio benchmark study of the H + CO --> HCO reaction.
    Woon DE
    J Chem Phys; 1996 Dec; 105(22):9921-6. PubMed ID: 11541750
    [TBL] [Abstract][Full Text] [Related]  

  • 5. Ab initio study of C + H3+ reactions.
    Talbi D; DeFrees DJ
    Chem Phys Lett; 1991 Apr; 179(1-2):165-8. PubMed ID: 11538494
    [TBL] [Abstract][Full Text] [Related]  

  • 6. Ab initio predictions on the rotational spectra of carbon-chain carbene molecules.
    Maluendes SA; McLean AD
    Chem Phys Lett; 1992 Dec; 200(5):511-7. PubMed ID: 11538408
    [TBL] [Abstract][Full Text] [Related]  

  • 7. Ab initio characterization of MgCCH, MgCCH+, and MgC2 and pathways to their formation in the interstellar medium.
    Woon DE
    Astrophys J; 1996 Jan; 456(2):602-10. PubMed ID: 11541464
    [TBL] [Abstract][Full Text] [Related]  

  • 8. A correlated ab initio study of the X2A1 and A2E states of MgCH3.
    Woon DE
    J Chem Phys; 1996 Jun; 104(23):9495-8. PubMed ID: 11541846
    [TBL] [Abstract][Full Text] [Related]  

  • 9. Astronomical identification of the C3H radical.
    Thaddeus P; Gottlieb CA; Hjalmarson A; Johansson LE; Irvine WM; Friberg P; Linke RA
    Astrophys J; 1985 Jul; 294(1):L49-53. PubMed ID: 11540839
    [TBL] [Abstract][Full Text] [Related]  

  • 10. A combined experimental and theoretical study on the formation of interstellar C3H isomers.
    Kaiser RI; Ochsenfeld C; Head-Gordon M; Lee YT; Suits AG
    Science; 1996 Nov; 274(5292):1508-11. PubMed ID: 8929407
    [TBL] [Abstract][Full Text] [Related]  

  • 11. The rate of the reaction between C2H and C2H2 at interstellar temperatures.
    Herbst E; Woon DE
    Astrophys J; 1997 Nov; 489(1):109-12. PubMed ID: 11541459
    [TBL] [Abstract][Full Text] [Related]  

  • 12. Calculations on the competition between association and reaction for C3H(+) + H2.
    Maluendes SA; McLean AD; Yamashita K; Herbst E
    J Chem Phys; 1993 Aug; 99(4):2812-20. PubMed ID: 11539504
    [TBL] [Abstract][Full Text] [Related]  

  • 13. Why HOC+ is detectable in interstellar clouds: the rate of the reaction between HOC+ and H2.
    Herbst E; Woon DE
    Astrophys J; 1996 Jun; 463(2):L113-5. PubMed ID: 11541463
    [TBL] [Abstract][Full Text] [Related]  

  • 14. A high-precision ab initio determination of the equilibrium geometry and force field of HOC+.
    DeFrees DJ; Bunker PR; Binkley JS; McLean AD
    J Mol Spectrosc; 1987; 121():440-9. PubMed ID: 11542123
    [TBL] [Abstract][Full Text] [Related]  

  • 15. Chemical evolution of circumstellar matter around young stellar objects.
    van Dishoeck EF; Blake GA
    Astrophys Space Sci; 1995; 224():237-49. PubMed ID: 11538416
    [TBL] [Abstract][Full Text] [Related]  

  • 16. A priori predictions of the rotational constants for HC13N, HC15N, C5O.
    DeFrees DJ; McLean AD
    Chem Phys Lett; 1989 Jun; 158(6):540-4. PubMed ID: 11542172
    [TBL] [Abstract][Full Text] [Related]  

  • 17. Theoretical prediction of the ionization energies of the C4H7 radicals: 1-methylallyl, 2-methylallyl, cyclopropylmethyl, and cyclobutyl radicals.
    Lau KC; Zheng W; Wong NB; Li WK
    J Chem Phys; 2007 Oct; 127(15):154302. PubMed ID: 17949144
    [TBL] [Abstract][Full Text] [Related]  

  • 18. Infrared laser spectroscopy of jet-cooled carbon clusters: the nu 5 band of linear C9.
    Van Orden A; Provencal RA; Keutsch FN; Saykally RJ
    J Chem Phys; 1996 Oct; 105(15):6111-6. PubMed ID: 11541745
    [TBL] [Abstract][Full Text] [Related]  

  • 19. Characterization of silicon-carbon clusters by infrared laser spectroscopy: the nu 3(sigma u) band of linear Si2C3.
    Van Orden A; Giesen TF; Provencal RA; Hwang HJ; Saykally RJ
    J Chem Phys; 1994 Dec; 101(12):10237-41. PubMed ID: 11539561
    [TBL] [Abstract][Full Text] [Related]  

  • 20. Ab initio calculation of electronic absorption spectra and ionization potentials of C3H3 radicals.
    Eisfeld W
    Phys Chem Chem Phys; 2005 Dec; 7(23):3924-32. PubMed ID: 19810320
    [TBL] [Abstract][Full Text] [Related]  

    [Next]    [New Search]
    of 6.