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Monthly Notices of the Royal Astronomical Society is a peer-reviewed journal published by Royal Astronomical Society, covering Stellar, planetary, and galactic studies, Galaxies: Formation, Evolution, Phenomena, Astrophysics and Star Formation Studies. Over its lifetime it has published 94,365 papers, which have received 3,638,727 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, 12(3), pp. 45–58.
Formats any DOI in the closest standard style — Monthly Notices of the Royal Astronomical Society has no published style definition, so this is an approximation. No sign-up. |
| Publishes research in | Stellar, planetary, and galactic studies Galaxies: Formation, Evolution, Phenomena Astrophysics and Star Formation Studies Astronomy and Astrophysical Research Astrophysical Phenomena and Observations |
| ISSN | 0035-8711 |
| Citation impact (2-yr) | 4.9 |
| h-index | 498 |
| i10-index | 56,674 |
| Article processing charge | $2,833 |
| Open access | Yes — indexed in DOAJ |
| Top institutions publishing here | Centre National de la Recherche Scientifique |
| Journal website | mnras.oxfordjournals.org |
| 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.
We present a new model for computing the spectral evolution of stellar populations at ages between 100,000 yr and 20 Gyr at a resolution of 3 A across the whole wavelength range from 3200 to 9500 A for a wide range of metallicities. These predictions are based on a newly available library of observed stellar…
(shortened) In this contribution an average or Galactic-field IMF is defined, stressing that there is evidence for a change in the power-law index at only two masses: near 0.5 Msun and 0.08 Msun. Using this supposed universal IMF, the uncertainty inherent to any observational estimate of the IMF is investigated, by studying the scatter introduced…
A new hydrodynamic code applicable to a space of an arbitrary number of dimensions is discussed and applied to a variety of polytropic stellar models. The principal feature of the method is the use of statistical techniques to recover analytical expressions for the physical variables from a known distribution of fluid elements. The equations of…
We discuss the cosmological simulation code GADGET-2, a new massively parallel TreeSPH code, capable of following a collisionless fluid with the N-body method, and an ideal gas by means of smoothed particle hydrodynamics (SPH). Our implementation of SPH manifestly conserves energy and entropy in regions free of dissipation, while allowing for fully adaptive smoothing lengths.…
When a rotating black hole is threaded by magnetic field lines supported by external currents flowing in an equatorial disc, an electric potential difference will be induced. If the field strength is large enough, the vacuum is unstable to a cascade production of electron–positron pairs and a surrounding force-free magnetosphere will be established. Under these…
