Results 161 to 170 of about 8,080,766 (192)

Efficient formation of a massive quiescent galaxy at redshift 4.9. [PDF]

Nat Astron
de Graaff A, Setton DJ, Brammer G, Cutler S, Suess KA, Labbé I, Leja J, Weibel A, Maseda MV, Whitaker KE, Bezanson R, Boogaard LA, Cleri NJ, De Lucia G, Franx M, Greene JE, Hirschmann M, Matthee J, McConachie I, Naidu RP, Oesch PA, Price SH, Rix HW, Valentino F, Wang B, Williams CC.   +25 more
europepmc   +1 more source

Pheno-morphological and biochemical characterization of root nodules and associated root nodulating bacteria from <i>Pongamia pinnata</i> (L.) Pierre in the arid regions of India. [PDF]

Front Plant Sci
Vyas V, Singh S, Choudhary S, Bhoi TK, Dey P, Saraswat A.   +5 more
europepmc   +1 more source

Computational approaches to modeling dynamos in galaxies. [PDF]

Living Rev Comput Astrophys
Korpi-Lagg MJ, Mac Low MM, Gent FA.
europepmc   +1 more source

The waning of the WIMP: endgame? [PDF]

Eur Phys J C Part Fields
Arcadi G, Cabo-Almeida D, Dutra M, Ghosh P, Lindner M, Mambrini Y, Neto JP, Pierre M, Profumo S, Queiroz FS.   +9 more
europepmc   +1 more source

Cosmology and fundamental physics with the ELT-ANDES spectrograph. [PDF]

Exp Astron (Dordr)
Martins CJAP, Cooke R, Liske J, Murphy MT, Noterdaeme P, Schmidt TM, Alcaniz JS, Alves CS, Balashev S, Cristiani S, Di Marcantonio P, Génova Santos R, Gonçalves RS, González Hernández JI, Maiolino R, Marconi A, Marques CMJ, Melo E Sousa MAF, Nunes NJ, Origlia L, Péroux C, Vinzl S, Zanutta A.   +22 more
europepmc   +1 more source

Bound star clusters observed in a lensed galaxy 460 Myr after the Big Bang. [PDF]

Nature
Adamo A, Bradley LD, Vanzella E, Claeyssens A, Welch B, Diego JM, Mahler G, Oguri M, Sharon K, Abdurro'uf, Hsiao TY, Xu X, Messa M, Lassen AE, Zackrisson E, Brammer G, Coe D, Kokorev V, Ricotti M, Zitrin A, Fujimoto S, Inoue AK, Resseguier T, Rigby JR, Jiménez-Teja Y, Windhorst RA, Hashimoto T, Tamura Y.   +27 more
europepmc   +1 more source

Analysis methods for Milky Way dark matter halo detection [PDF]

AIP Conference Proceedings, 2007
We present methods for the analysis of dark matter annihilation in the smooth halo of the Milky Way galaxy. We model the diffuse gamma-ray background using GALPROP, and model the halo using an NFW profile and the gamma-ray spectrum for WIMP pair annihilation.
Igor Moskalenko, Brian Winer
exaly   +4 more sources

CONSTRAINTS ON THE SHAPE OF THE MILKY WAY DARK MATTER HALO FROM THE SAGITTARIUS STREAM [PDF]

Astrophysical Journal Letters, 2013
We propose a new model for the dark matter halo of the Milky Way that fits the properties of the stellar stream associated with the Sagittarius dwarf galaxy. Our dark halo is oblate with q_z = 0.9 for r < 10 kpc, and can be made to follow the Law & Majewski model at larger radii.
Carlos Vera-Ciro, Amina Helmi
exaly   +5 more sources

On the edge: the relation between stellar and dark matter haloes of Milky Way-mass galaxies [PDF]

Monthly Notices of the Royal Astronomical Society, 2023
We investigate the build-up of the accreted stellar and dark matter haloes of Milky Way-like galaxies in APOSTLE suite of cosmological hydrodynamics simulations.
Alis Deason, Carlos Frenk, Anna Genina
exaly   +2 more sources

Warm dark matter constraints using Milky Way satellite observations and subhalo evolution modeling [PDF]

Physical Review D, 2022
Warm dark matter (WDM) can potentially explain small-scale observations that currently challenge the cold dark matter (CDM) model, as warm particles suppress structure formation due to free-streaming effects.
Shin'ichiro Ando, Kenny C Y Ng, Ariane Dekker   +2 more
exaly   +3 more sources