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 *

388 related articles for article (PubMed ID: 11882889)

  • 1. Massive star formation in 100,000 years from turbulent and pressurized molecular clouds.
    McKee CF; Tan JC
    Nature; 2002 Mar; 416(6876):59-61. PubMed ID: 11882889
    [TBL] [Abstract][Full Text] [Related]  

  • 2. A minimum column density of 1 g cm(-2) for massive star formation.
    Krumholz MR; McKee CF
    Nature; 2008 Feb; 451(7182):1082-4. PubMed ID: 18305539
    [TBL] [Abstract][Full Text] [Related]  

  • 3. The formation of a massive protostar through the disk accretion of gas.
    Chini R; Hoffmeister V; Kimeswenger S; Nielbock M; Nürnberger D; Schmidtobreick L; Sterzik M
    Nature; 2004 May; 429(6988):155-7. PubMed ID: 15141204
    [TBL] [Abstract][Full Text] [Related]  

  • 4. 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]  

  • 5. A substantial population of low-mass stars in luminous elliptical galaxies.
    van Dokkum PG; Conroy C
    Nature; 2010 Dec; 468(7326):940-2. PubMed ID: 21124316
    [TBL] [Abstract][Full Text] [Related]  

  • 6. The essential signature of a massive starburst in a distant quasar.
    Solomon P; Vanden Bout P; Carilli C; Guelin M
    Nature; 2003 Dec; 426(6967):636-8. PubMed ID: 14668856
    [TBL] [Abstract][Full Text] [Related]  

  • 7. Fragmentation in massive star formation.
    Beuther H; Schilke P
    Science; 2004 Feb; 303(5661):1167-9. PubMed ID: 14976307
    [TBL] [Abstract][Full Text] [Related]  

  • 8. Infall of gas as the formation mechanism of stars up to 20 times more massive than the Sun.
    Beltrán MT; Cesaroni R; Codella C; Testi L; Furuya RS; Olmi L
    Nature; 2006 Sep; 443(7110):427-9. PubMed ID: 17006508
    [TBL] [Abstract][Full Text] [Related]  

  • 9. Clustered star formation and the origin of stellar masses.
    Pudritz RE
    Science; 2002 Jan; 295(5552):68-76. PubMed ID: 11778037
    [TBL] [Abstract][Full Text] [Related]  

  • 10. Star formation around supermassive black holes.
    Bonnell IA; Rice WK
    Science; 2008 Aug; 321(5892):1060-2. PubMed ID: 18719276
    [TBL] [Abstract][Full Text] [Related]  

  • 11. Energy input from quasars regulates the growth and activity of black holes and their host galaxies.
    Di Matteo T; Springel V; Hernquist L
    Nature; 2005 Feb; 433(7026):604-7. PubMed ID: 15703739
    [TBL] [Abstract][Full Text] [Related]  

  • 12. The initial mass function of stars: evidence for uniformity in variable systems.
    Kroupa P
    Science; 2002 Jan; 295(5552):82-91. PubMed ID: 11778039
    [TBL] [Abstract][Full Text] [Related]  

  • 13. Habitable zones exposed: astrosphere collapse frequency as a function of stellar mass.
    Smith DS; Scalo JM
    Astrobiology; 2009 Sep; 9(7):673-81. PubMed ID: 19778278
    [TBL] [Abstract][Full Text] [Related]  

  • 14. Early turbulent mixing as the origin of chemical homogeneity in open star clusters.
    Feng Y; Krumholz MR
    Nature; 2014 Sep; 513(7519):523-5. PubMed ID: 25174709
    [TBL] [Abstract][Full Text] [Related]  

  • 15. The formation of massive star systems by accretion.
    Krumholz MR; Klein RI; McKee CF; Offner SS; Cunningham AJ
    Science; 2009 Feb; 323(5915):754-7. PubMed ID: 19150809
    [TBL] [Abstract][Full Text] [Related]  

  • 16. Spherical episodic ejection of material from a young star.
    Torrelles JM; Patel NA; Gómez JF; Ho PT; Rodríguez LF; Anglada G; Garay G; Greenhill L; Curiel S; Cantó J
    Nature; 2001 May; 411(6835):277-80. PubMed ID: 11357123
    [TBL] [Abstract][Full Text] [Related]  

  • 17. Formation of new stellar populations from gas accreted by massive young star clusters.
    Li C; de Grijs R; Deng L; Geller AM; Xin Y; Hu Y; Faucher-Giguère CA
    Nature; 2016 Jan; 529(7587):502-4. PubMed ID: 26819043
    [TBL] [Abstract][Full Text] [Related]  

  • 18. A circumstellar disk associated with a massive protostellar object.
    Jiang Z; Tamura M; Fukagawa M; Hough J; Lucas P; Suto H; Ishii M; Yang J
    Nature; 2005 Sep; 437(7055):112-5. PubMed ID: 16136137
    [TBL] [Abstract][Full Text] [Related]  

  • 19. The formation of stellar systems from interstellar molecular clouds.
    Gehrz RD; Black DC; Solomon PM
    Science; 1984 May; 224(4651):823-30. PubMed ID: 17743183
    [TBL] [Abstract][Full Text] [Related]  

  • 20. Accretion of low-metallicity gas by the Milky Way.
    Wakker BP; Howk JC; Savage BD; van Woerden H; Tufte SL; Schwarz UJ; Benjamin R; Reynolds RJ; Peletier RF; Kalberla PM
    Nature; 1999 Nov; 402(6760):388-90. PubMed ID: 10586877
    [TBL] [Abstract][Full Text] [Related]  

    [Next]    [New Search]
    of 20.