Results 221 to 230 of about 144,718 (240)
JWST detection of heavy neutron capture elements in a compact object merger
, 2023 Levan A, Gompertz B, Salafia OS, Bulla M, Burns E, Hotokezaka K, Izzo L, Lamb G, Malesani D, Oates S, Ravasio M, Escorial AR, Schneider B, Sarin N, Schulze S, Tanvir N, Ackley K, Anderson G, Brammer G, Christensen L, Dhillon V, Evans P, Fausnaugh M, Fong W, Fruchter A, Fryer C, Fynbo J, Gaspari N, Heintz K, Hjorth J, Kennea J, Kennedy M, Laskar T, Leloudas G, Mandel I, Martín-Carrillo A, Metzger B, Nicholl M, Nugent A, Palmerio J, Pugilese G, Rastinejad J, Rhodes L, Rossi A, Smartt S, Stevance H, Tohuvavohu A, Horst Avd, Vergani S, Watson D, Barclay T, Bhirombhakdi K, Breedt E, Breeveld A, Brown A, Campana S, D'Avanzo P, D'Elia V, De Pasquale M, Dyer M, Galloway D, Garbutt J, Green M, Hartmann D, Jakobsson P, Kerry P, Langeroodi D, Leung J, Littlefair S, Munday J, O'Brien P, Parsons S, Pelisoli I, Sahman D, Salvaterra R, Tagliaferri G, Thöne C, Postigo AdU, Sbarufatti B, Chrimes A, Steeghs D, Kann D. +81 moreeuropepmc +1 more sourceHeavy-element production in a compact object merger observed by JWST. [PDF]
NatureLevan AJ, Gompertz BP, Salafia OS, Bulla M, Burns E, Hotokezaka K, Izzo L, Lamb GP, Malesani DB, Oates SR, Ravasio ME, Rouco Escorial A, Schneider B, Sarin N, Schulze S, Tanvir NR, Ackley K, Anderson G, Brammer GB, Christensen L, Dhillon VS, Evans PA, Fausnaugh M, Fong WF, Fruchter AS, Fryer C, Fynbo JPU, Gaspari N, Heintz KE, Hjorth J, Kennea JA, Kennedy MR, Laskar T, Leloudas G, Mandel I, Martin-Carrillo A, Metzger BD, Nicholl M, Nugent A, Palmerio JT, Pugliese G, Rastinejad J, Rhodes L, Rossi A, Saccardi A, Smartt SJ, Stevance HF, Tohuvavohu A, van der Horst A, Vergani SD, Watson D, Barclay T, Bhirombhakdi K, Breedt E, Breeveld AA, Brown AJ, Campana S, Chrimes AA, D'Avanzo P, D'Elia V, De Pasquale M, Dyer MJ, Galloway DK, Garbutt JA, Green MJ, Hartmann DH, Jakobsson P, Kerry P, Kouveliotou C, Langeroodi D, Le Floc'h E, Leung JK, Littlefair SP, Munday J, O'Brien P, Parsons SG, Pelisoli I, Sahman DI, Salvaterra R, Sbarufatti B, Steeghs D, Tagliaferri G, Thöne CC, de Ugarte Postigo A, Kann DA. +84 moreeuropepmc +1 more sourceQuasi-periodic X-ray eruptions years after a nearby tidal disruption event. [PDF]
NatureNicholl M, Pasham DR, Mummery A, Guolo M, Gendreau K, Dewangan GC, Ferrara EC, Remillard R, Bonnerot C, Chakraborty J, Hajela A, Dhillon VS, Gillan AF, Greenwood J, Huber ME, Janiuk A, Salvesen G, van Velzen S, Aamer A, Alexander KD, Angus CR, Arzoumanian Z, Auchettl K, Berger E, de Boer T, Cendes Y, Chambers KC, Chen TW, Chornock R, Fulton MD, Gao H, Gillanders JH, Gomez S, Gompertz BP, Fabian AC, Herman J, Ingram A, Kara E, Laskar T, Lawrence A, Lin CC, Lowe TB, Magnier EA, Margutti R, McGee SL, Minguez P, Moore T, Nathan E, Oates SR, Patra KC, Ramsden P, Ravi V, Ridley EJ, Sheng X, Smartt SJ, Smith KW, Srivastav S, Stein R, Stevance HF, Turner SGD, Wainscoat RJ, Weston J, Wevers T, Young DR. +63 moreeuropepmc +1 more sourceThe Rotation of Spiral Galaxies [PDF]
Science, 1983 There is accumulating evidence that as much as 90 percent of the mass of the universe is nonluminous and is clumped, halo-like, around individual galaxies. The gravitational force of this dark matter is presumed to be responsible for the high rotational velocities of stars and gas in the disks of spiral galaxies.openaire +2 more sourcesOpaque spiral galaxies [PDF]
Nature, 1990 The photographic images of a carefully selected sample of about 16,000 galaxies have been digitized, and an extensive set of photometric parameters has been determined. These data allow a reanalysis of the effective transparency using the measured surface brightness profiles for much larger, more strictly defined samples. Several tests provide evidence openaire +2 more sources
