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PUBMED FOR HANDHELDS

Journal Abstract Search


140 related items for PubMed ID: 21673671

  • 21. Heart of a stellar explosion revealed.
    Nakar E.
    Nature; 2019 Jan; 565(7739):300-301. PubMed ID: 30651620
    [No Abstract] [Full Text] [Related]

  • 22. A strong ultraviolet pulse from a newborn type Ia supernova.
    Cao Y, Kulkarni SR, Howell DA, Gal-Yam A, Kasliwal MM, Valenti S, Johansson J, Amanullah R, Goobar A, Sollerman J, Taddia F, Horesh A, Sagiv I, Cenko SB, Nugent PE, Arcavi I, Surace J, Woźniak PR, Moody DI, Rebbapragada UD, Bue BD, Gehrels N.
    Nature; 2015 May 21; 521(7552):328-31. PubMed ID: 25993962
    [Abstract] [Full Text] [Related]

  • 23. Planetary nebulae: understanding the physical and chemical evolution of dying stars.
    Weinberger R, Kerber F.
    Science; 1997 May 30; 276(5317):1382-6. PubMed ID: 9161999
    [Abstract] [Full Text] [Related]

  • 24. Cosmic rays from nearby supernovae: biological effects.
    Laster H.
    Science; 1968 Jun 07; 160(3832):1138. PubMed ID: 5647438
    [No Abstract] [Full Text] [Related]

  • 25. Mechanism for spectral break in cosmic ray proton spectrum of supernova remnant W44.
    Malkov MA, Diamond PH, Sagdeev RZ.
    Nat Commun; 2011 Feb 15; 2():194. PubMed ID: 21326226
    [Abstract] [Full Text] [Related]

  • 26. Cosmic rays from nearby supernovae: biological effects.
    Tucker WH, Terry KD.
    Science; 1968 Jun 07; 160(3832):1138-9. PubMed ID: 5647439
    [No Abstract] [Full Text] [Related]

  • 27. Bridging the gap: from massive stars to supernovae.
    Maund JR, Crowther PA, Janka HT, Langer N.
    Philos Trans A Math Phys Eng Sci; 2017 Oct 28; 375(2105):. PubMed ID: 28923995
    [Abstract] [Full Text] [Related]

  • 28. Cosmic vacuum energy decay and creation of cosmic matter.
    Fahr HJ, Heyl M.
    Naturwissenschaften; 2007 Sep 28; 94(9):709-24. PubMed ID: 17457553
    [Abstract] [Full Text] [Related]

  • 29. Indirect techniques in nuclear astrophysics: a review.
    Tribble RE, Bertulani CA, Cognata ML, Mukhamedzhanov AM, Spitaleri C.
    Rep Prog Phys; 2014 Oct 28; 77(10):106901. PubMed ID: 25313189
    [Abstract] [Full Text] [Related]

  • 30. A large oxygen-dominated core from the seismic cartography of a pulsating white dwarf.
    Giammichele N, Charpinet S, Fontaine G, Brassard P, Green EM, Van Grootel V, Bergeron P, Zong W, Dupret MA.
    Nature; 2018 Feb 01; 554(7690):73-76. PubMed ID: 29310123
    [Abstract] [Full Text] [Related]

  • 31. No signature of ejecta interaction with a stellar companion in three type Ia supernovae.
    Olling RP, Mushotzky R, Shaya EJ, Rest A, Garnavich PM, Tucker BE, Kasen D, Margheim S, Filippenko AV.
    Nature; 2015 May 21; 521(7552):332-5. PubMed ID: 25993963
    [Abstract] [Full Text] [Related]

  • 32. Cosmology with cosmic shear observations: a review.
    Kilbinger M.
    Rep Prog Phys; 2015 Jul 21; 78(8):086901. PubMed ID: 26181770
    [Abstract] [Full Text] [Related]

  • 33. 'Let the stars shine in peace!' Niels Bohr and stellar energy, 1929-1934.
    Kragh H.
    Ann Sci; 2017 Apr 21; 74(2):126-148. PubMed ID: 28492099
    [Abstract] [Full Text] [Related]

  • 34. Physical mechanism of core-collapse supernovae that neutrinos drive.
    Yamada S, Nagakura H, Akaho R, Harada A, Furusawa S, Iwakami W, Okawa H, Matsufuru H, Sumiyoshi K.
    Proc Jpn Acad Ser B Phys Biol Sci; 2024 Apr 21; 100(3):190-233. PubMed ID: 38462501
    [Abstract] [Full Text] [Related]

  • 35. Gamma and neutrino radiation dose from gamma ray bursts and nearby supernovae.
    Karam PA.
    Health Phys; 2002 Apr 21; 82(4):491-9. PubMed ID: 11906138
    [Abstract] [Full Text] [Related]

  • 36. Circumstellar material in type Ia supernovae via sodium absorption features.
    Sternberg A, Gal-Yam A, Simon JD, Leonard DC, Quimby RM, Phillips MM, Morrell N, Thompson IB, Ivans I, Marshall JL, Filippenko AV, Marcy GW, Bloom JS, Patat F, Foley RJ, Yong D, Penprase BE, Beeler DJ, Allende Prieto C, Stringfellow GS.
    Science; 2011 Aug 12; 333(6044):856-9. PubMed ID: 21836010
    [Abstract] [Full Text] [Related]

  • 37. Newly formed dust within the circumstellar environment of SN Ia-CSM 2018evt.
    Wang王 L灵, Hu M, Wang L, Yang 杨 Y轶, Yang J, Gomez H, Chen S, Hu L, Chen TW, Mo J, Wang X, Baade D, Hoeflich P, Wheeler JC, Pignata G, Burke J, Hiramatsu D, Howell DA, McCully C, Pellegrino C, Galbany L, Hsiao EY, Sand DJ, Zhang J, Uddin SA, Anderson JP, Ashall C, Cheng C, Gromadzki M, Inserra C, Lin H, Morrell N, Morales-Garoffolo A, Müller-Bravo TE, Nicholl M, Gonzalez EP, Phillips MM, Pineda-García J, Sai H, Smith M, Shahbandeh M, Srivastav S, Stritzinger MD, Yang S, Young DR, Yu L, Zhang X.
    Nat Astron; 2024 Aug 12; 8(4):504-519. PubMed ID: 38659610
    [Abstract] [Full Text] [Related]

  • 38. Evidence for two distinct populations of type Ia supernovae.
    Wang X, Wang L, Filippenko AV, Zhang T, Zhao X.
    Science; 2013 Apr 12; 340(6129):170-3. PubMed ID: 23470733
    [Abstract] [Full Text] [Related]

  • 39. The Explosion and Progenitor Properties of Type IIP Supernovae Inferred from MESA and STELLA Modelling.
    Ricks W, Dwarkadas VV.
    Res Notes AAS; 2020 Jul 12; 4(7):. PubMed ID: 33354654
    [Abstract] [Full Text] [Related]

  • 40. Risk from supernovae compared wth risk standards for nuclear reactors.
    Bowen JH.
    Nature; 1968 Oct 19; 220(5164):303-4. PubMed ID: 5684867
    [No Abstract] [Full Text] [Related]


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