Results 101 to 110 of about 59,474 (295)

The chemical evolution of galaxy clusters: Dissecting the iron mass budget of the intracluster medium [PDF]

, 2020
Ang Liu, Paolo Tozzi, Stefano Ettori, Sabrina De Grandi, Fabio Gastaldello, Piero Rosati, Colin Norman   +6 more
openalex   +1 more source

Forensic analysis and evaluation of file‐wiping applications in Android OS

Journal of Forensic Sciences, EarlyView.
Abstract Anti‐forensics refers to techniques designed to obstruct the discovery of evidence in digital forensic investigations. File‐wiping is one of the anti‐forensic techniques that make data recovery impossible by overwriting data with specific patterns. This technique poses significant challenges to investigators.
Dong Bin Oh, Somi Lim, Suji Lee, Yesong Jo, Gahyun Choi, Bumyun Kim, Huy Kang Kim   +6 more
wiley   +1 more source

Unveiling the Galactic Baryon Cycle Process by an Empirical Model

The Astrophysical Journal
We propose an empirical model to describe and constrain the baryon cycle process during galaxy evolution. This model utilizes the evolution of star formation rate, derived from the stellar mass–halo mass relations across different redshifts, and the cold
Yaoxin Chen, Xi Kang, Hong Guo, Hou-Zun Chen, Jiafeng Lu   +4 more
doaj   +1 more source

Chemical Evolution of the Galaxy

, 1994
ten pages in CUPstyle LaTex: extract at the end the corresponding confguid ...
openaire   +2 more sources

Chemical evolution of galaxies and galaxy formation mechanisms [PDF]

Proceedings of Baryons in Dark Matter Halos — PoS(BDMH2004), 2004
I will describe the results if models for the chemical evolution of galaxies of different morphological type (ellipticals, spirals and irregulars), and compare them with observations in order to impose constraints on the mechianisms of formation and evolution of galaxies.
openaire   +1 more source

Chromosome‐scale genome assembly of the South American fruit fly, Anastrepha fraterculus sp.1

Insect Science, EarlyView.
Anastrepha fraterculus sp. 1 is a major fruit fly pest in Argentina, currently controlled through chemical treatments and traps. This study aims to enhance the genomic understanding of this species to support the development of sterile insect technique as well as the use of innovative technologies.
Máximo Rivarola, Claudia A. Conte, Pierre Berube, Shu‐Huang Chen, M. Cecilia Giardini, Alejandra C. Scannapieco, Fabián H. Milla, María C. Soria, Romina M. Russo, Juan P. Wulff, Haig H. Djambazian, Rolando R. Pomar, Alfred M. Handler, Kostas Bourtzis, Ioannis Ragoussis, Silvia B. Lanzavecchia   +15 more
wiley   +1 more source

Low [O/Fe] Ratio in a Luminous Galaxy at the Early Cosmic Epoch (z > 10): Signature of Short Delay Time or Bright Hypernovae/Pair-instability Supernovae?

The Astrophysical Journal
We present an [O/Fe] ratio of a luminous galaxy GN-z11 at z = 10.60 derived with the deep public JWST/NIRSpec data. We fit the medium-resolution grating (G140M, G235M, and G395M) data with the model spectra consisting of BPASS-stellar and Cloudy -nebular
Minami Nakane, Masami Ouchi, Kimihiko Nakajima, Yuichi Harikane, Nozomu Tominaga, Koh Takahashi, Daichi Kashino, Hiroto Yanagisawa, Kuria Watanabe, Ken’ichi Nomoto, Yuki Isobe, Moka Nishigaki, Miho N. Ishigaki, Yoshiaki Ono, Yui Takeda   +14 more
doaj   +1 more source

Chemical enrichment of galaxy clusters from hydrodynamical simulations

, 2007
We present cosmological hydrodynamical simulations of galaxy clusters aimed at studying the process of metal enrichment of the intra--cluster medium (ICM).
Arimoto, Balestra, Bate, Baumgartner, Bertelli, Borgani, Cen, Chiappini, Chiappini, Chieffi, Cora, Dalla Vecchia, Davé, De Grandi, De Lucia, Dolag, Domainko, F. Matteucci, Finoguenov, Finoguenov, François, Gal-Yam, Gal-Yam, Gastaldello, Gibson, Greggio, Haardt, Iwamoto, K. Dolag, Katz, Kawata, Kay, Kennicutt, Kobayashi, Kroupa, L. Tornatore, Larson, Lia, Loewenstein, Maeder, Maoz, Marigo, Matteucci, Matteucci, Matteucci, Matteucci, Matteucci, Mazzotta, Monaco, Mosconi, Murante, Mushotzky, Nagashima, Navarro, Padovani, Pipino, Portinari, Portinari, Raiteri, Rasia, Rasia, Rebusco, Recchi, Renzini, Renzini, Renzini, Roediger, Romano, Romeo, Rosati, S. Borgani, Salpeter, Samland, Sarazin, Saro, Scalo, Scannapieco, Scannapieco, Schmidt, Sijacki, Sijacki, Sommer-Larsen, Springel, Springel, Springel, Springel, Springel, Springel, Strickland, Sutherland, Tamura, Theis, Thielemann, Tormen, Tornatore, Tutukov, Valdarnini, Van Den Hoek, Vikhlinin, Vikhlinin, Voit, Woosley, Yoshikawa   +102 more
core   +2 more sources

The chemical evolution of galaxies

Metals -- heavy elements synthesized during various phases of stellar evolution or during supernova explosions -- play a fundamental role in shaping galaxy evolution. In fact, their relative abundances, spatial distribution, and scaling with galactic properties reflect the constant interplay between star-formation, nucleosynthesis, and gas flows that ...
openaire   +2 more sources

The Chemical Evolution of Galaxies by Successive Starbursts

, 1999
We propose an evolutionary scenario by successive bursts of star formation to reproduce the chemical properties of massive nearby Starburst Nucleus Galaxies (SBNGs). The N/O abundance ratios in SBNGs are 0.2 dex higher than in normal HII regions observed in the disks of late-type spirals.
Contini, T., Coziol, R., Considère, S., Davoust, E., Reyes, R.E. Carlos   +4 more
openaire   +3 more sources