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Monthly Notices of the Royal Astronomical Society: Letters is a peer-reviewed journal published by Royal Astronomical Society, covering Galaxies: Formation, Evolution, Phenomena, Stellar, planetary, and galactic studies, Astrophysics and Star Formation Studies. Over its lifetime it has published 3,863 papers, which have received 151,129 citations.
| Publisher | Royal Astronomical Society |
|---|---|
| Reference style | Author–year (MNRAS) Author–year — (Smith, 2023) in the text Smith, A., Jones, B. and Lee, C. (2023) 'A representative article title', Monthly Notices of the Royal Astronomical Society: Letters, 12(3), pp. 45–58.
Formats any DOI in the closest standard style — Monthly Notices of the Royal Astronomical Society: Letters has no published style definition, so this is an approximation. No sign-up. |
| Publishes research in | Galaxies: Formation, Evolution, Phenomena Stellar, planetary, and galactic studies Astrophysics and Star Formation Studies Astrophysical Phenomena and Observations Gamma-ray bursts and supernovae |
| ISSN | 1745-3925 |
| Citation impact (2-yr) | 5.46 |
| h-index | 143 |
| i10-index | 2,823 |
| Article processing charge | $2,833 |
| Top institutions publishing here | Centre National de la Recherche Scientifique |
| Journal website | academic.oup.com |
| You get | A submission-ready PDF and the editable LaTeX source — ready to submit. |
Citations each year’s papers have accumulated so far — the most recent years are still building up.
Abstract We show that dissipationless Λ cold dark matter simulations predict that the majority of the most massive subhaloes of the Milky Way are too dense to host any of its bright satellites (LV > 105 L⊙). These dark subhaloes have peak circular velocities at infall of Vinfall= 30–70 km s-1 and infall masses of…
ABSTRACT We describe global, 3D, time-dependent, non-radiative, general-relativistic, magnetohydrodynamic simulations of accreting black holes (BHs). The simulations are designed to transport a large amount of magnetic flux to the centre, more than the accreting gas can force into the BH. The excess magnetic flux remains outside the BH, impedes accretion, and leads to a magnetically…
Abstract One of the most compelling tasks of modern cosmology is to constrain the expansion history of the Universe, since this measurement can give insights on the nature of dark energy and help to estimate cosmological parameters. In this letter are presented two new measurements of the Hubble parameter H(z) obtained with the cosmic chronometer…
Abstract Model selection is the problem of distinguishing competing models, perhaps featuring different numbers of parameters. The statistics literature contains two distinct sets of tools, those based on information theory such as the Akaike Information Criterion (AIC), and those on Bayesian inference such as the Bayesian evidence and Bayesian Information Criterion (BIC). The Deviance Information…
Abstract We use a combination of three large N-body simulations to investigate the dependence of dark matter halo concentrations on halo mass and redshift in the Wilkinson Microwave Anisotropy Probe year 5 (WMAP5) cosmology. The median relation between concentration and mass is adequately described by a power law for halo masses in the range 1011–1015h−1…
