화학공학소재연구정보센터
검색결과 : 4건
No. Article
1 A recurrent nova super-remnant in the Andromeda galaxy
Darnley MJ, Hounsell R, O'Brien TJ, Henze M, Rodriguez-Gil P, Shafter AW, Shara MM, Vaytet NMH, Bode MF, Ciardullo R, Davis BD, Galera-Rosillo R, Harman DJ, Harvey EJ, Healy MW, Ness JU, Ribeiro VARM, Williams SC
Nature, 565(7740), 460, 2019
2 Proper-motion age dating of the progeny of Nova Scorpii ad 1437
Shara MM, Ilkiewicz K, Mikolajewska J, Pagnotta A, Bode MF, Crause LA, Drozd K, Faherty J, Fuentes-Morales I, Grindlay JE, Moffat AFJ, Pretorius ML, Schmidtobreick L, Stephenson FR, Tappert C, Zurek D
Nature, 548(7669), 558, 2017
3 An age difference of two billion years between a metal-rich and a metal-poor globular cluster
Hansen BMS, Kalirai JS, Anderson J, Dotter A, Richer HB, Rich RM, Shara MM, Fahlman GG, Hurley JR, King IR, Reitzel D, Stetson PB
Nature, 500(7460), 51, 2013
4 Exclusion of a luminous red giant as a companion star to the progenitor of supernova SN 2011fe
Li WD, Bloom JS, Podsiadlowski P, Miller AA, Cenko SB, Jha SW, Sullivan M, Howell DA, Nugent PE, Butler NR, Ofek EO, Kasliwal MM, Richards JW, Stockton A, Shih HY, Bildsten L, Shara MM, Bibby J, Filippenko AV, Ganeshalingam M, Silverman JM, Kulkarni SR, Law NM, Poznanski D, Quimby RM, McCully C, Patel B, Maguire K, Shen KJ
Nature, 480(7377), 348, 2011