Monthly Notices of the Royal Astronomical Society (MNRAS) is a peer-reviewed scientific journal covering research in astronomy and astrophysics. It has been in continuous existence since 1827 and publishes letters and papers reporting original research in relevant fields. Despite the name, the journal is no longer monthly, nor does it carry the notices of the Royal Astronomical Society.
|Monthly Notices of the Royal Astronomical Society|
|Edited by||David Flower|
|Monthly Notices of the Astronomical Society of London|
|Hybrid and delayed|
|Mon. Notices Royal Astron. Soc.|
|Mon Not R Astron Soc|
The first issue of MNRAS was published on 9 February 1827 as Monthly Notices of the Astronomical Society of London and it has been in continuous publication ever since. It took its current name from the second volume, after the Astronomical Society of London became the Royal Astronomical Society (RAS). Until 1960 it carried the monthly notices of the RAS, at which time these were transferred to the newly established Quarterly Journal of the Royal Astronomical Society (1960–1996) and then to its successor journal Astronomy & Geophysics (since 1997). Until 1965, MNRAS was published in-house by the society; from 1965 to 2012 it was published by Blackwell Publishing (later part of Wiley-Blackwell) on behalf of the RAS. From 2013, MNRAS is published by Oxford University Press (OUP).
The journal is no longer monthly, with thirty-six issues a year divided into nine volumes.
MNRAS publishes peer-reviewed articles on original research in astronomy and astrophysics. Two sorts of article are carried by MNRAS: papers, which can be of any length, and letters, which are published more quickly but are limited to five pages in length. Letters used to appear on pink pages in the print edition of the journal, but are now only published in full in the online edition with a contents list in the print edition. Editorial control of the journal is exercised by the RAS through an editorial board of professional astronomers; As of July 2012, the editor-in-chief is David Flower (University of Durham).
The stated policy of the RAS is "to focus on high quality papers through rigorous peer review and, as far as practicable, to provide free publication". Authors are not charged for publishing in MNRAS, with the costs of publications being met by subscriptions. MNRAS provides a form of open access by providing authors with the option to pay for publication, allowing free access by anyone without charge (hybrid open-access model). Fellows of the RAS are given free online access to the RAS journals as part of their membership benefits. Downloadable PDF versions of MNRAS articles are made available 36 months after publication (delayed open-access model), on both the journal website and the Astrophysics Data System. MNRAS also permits self-archiving by authors on personal webpages, in institutional repositories, and on the arXiv server (green open access). Also, authors are provided with a link to a perpetually freely accessible PDF file, the idea being that the file itself should not be hosted by the author nor by anyone except the publisher, while the link to it can be freely distributed. This is the modern equivalent of offprints, paper copies of the article which used to be provided to the author to distribute, freely, as he or she saw fit. Authors do not assign copyright to the RAS or OUP, but are required to grant an exclusive licence to publish the article prior to its publication.
The following persons have served as Editor-in-Chief (formerly titled Managing Editor or simply Editor):
The journal is abstracted and indexed in:
2002 VE68, also written 2002 VE68, is a temporary quasi-satellite of Venus. It was the first quasi-satellite to be discovered around a major planet in the Solar System. In a frame of reference rotating with Venus, it appears to travel around it during one Venerean year but it actually orbits the Sun, not Venus.41 Cygni
41 Cygni (41 Cyg) is a star in the constellation Cygnus. Its apparent magnitude is 4.02.45 Draconis
45 Draconis is a single star located in the northern circumpolar constellation of Draco, around 3,500 light years from the Earth. 45 Draconis is the Flamsteed designation, while it has the Bayer designation of d Draconis. This object is visible to the naked eye as a faint, yellow-white hued star with an apparent visual magnitude of 4.78. Radial velocity measurements indicate it is moving closer to the Sun at the rate of −12.5 km/s.Lyubimkov et al. (2012) assigned this star a stellar classification of F7Ib, matching an F-type supergiant. It is approximately 33 million years old with 8.2 times the mass of the Sun and about 62 times the Sun's radius. The star is radiating 5,450 times the Sun's luminosity from its photosphere at an effective temperature of 6,151 K.Alan Duffy (astronomer)
Alan R Duffy (born 1983) is a professional astronomer and science communicator. He was born in England, raised in Ireland, and is currently based in Australia. He is a Research Fellow and Associate Professor at the Centre for Astrophysics and Supercomputing at Swinburne University of Technology, and he is the Lead Scientist at the Royal Institution of Australia.
His research is focused on using super-computers to build and test models of the growth of galaxies within vast dark matter halos, and in particular focuses on the formation of the first galaxies in the early universe during the "Epoch of Reionisation". These models aim to improve our understanding of the nature of dark matter, and the large scale properties of the universe.Arthur Robert Hinks
Arthur Robert Hinks, CBE, FRS (26 May 1873 – 14 April 1945) was a British astronomer and geographer.As an astronomer, he is best known for his work in determining the distance from the Sun to the Earth (the astronomical unit) from 1900–1909: for this achievement, he was awarded the Gold Medal of the Royal Astronomical Society and was elected a fellow of the Royal Society. His later professional career was in surveying and cartography, an extension of his astronomical interests.F Hydrae
F Hydrae, also known as HD 74395, is a star in the constellation Hydra with an apparent magnitude is 4.64. It was catalogued as 31 Monocerotis, but this name is now rarely used since the star is now within the boundaries of Hydra. It is a low mass yellow supergiant around a thousand times brighter than the sun and five times as massive.
F Hya is a catalogued as a triple star, with 8th magnitude BD-06°2707 80" away and 13th magnitude companion at 57".Geophysical Journal International
Geophysical Journal International is a monthly peer-reviewed scientific journal published by Oxford University Press on behalf of the Royal Astronomical Society and the Deutsche Geophysikalische Gesellschaft (German Geophysical Society). The journal publishes original research papers, research notes, letters, and book reviews. It was established in 1922. The editor-in-chief is Joerg Renner (Ruhr University Bochum). The journal covers research on all aspects of theoretical, computational, applied and observational geophysics.List of most massive black holes
This is an ordered list of the most massive black holes so far discovered (and probable candidates), measured in units of solar masses (M☉), or the mass of the Sun (approx. 2×1030 kilograms).NGC 3665
NGC 3665 is a lenticular galaxy located in the constellation Ursa Major. It is located at a distance of circa 85 million light years from Earth, which, given its apparent dimensions, means that NGC 3665 is about 85,000 light years across. It was discovered by William Herschel on March 23, 1789.NGC 4111
NGC 4111 is a lenticular galaxy in the constellation Canes Venatici. It is located at a distance of circa 50 million light years from Earth, which, given its apparent dimensions, means that NGC 4111 is about 55,000 light years across. It was discovered by William Herschel in 1788.NGC 4494
NGC 4494 is an elliptical galaxy located in the constellation Coma Berenices. It is located at a distance of circa 45 million light years from Earth, which, given its apparent dimensions, means that NGC 4494 is about 60,000 light years across. It was discovered by William Herschel in 1785.NGC 4570
NGC 4570 is an edge-on lenticular galaxy located about 57 million light-years away in the constellation Virgo. NGC 4570 was discovered by astronomer William Herschel on April 13, 1784 and is a member of the Virgo Cluster.NGC 4709
NGC 4709 is an elliptical galaxy located in the constellation Centaurus. It is considered to be a member of the Centaurus Cluster and is the dominant member of a small group of galaxies known as "Cen 45" which is currently merging with the main Centaurus Cluster (Cen 30) even though the two subclusters' line of sight redshift velocities differ by about 1500 km/s. NGC 4709 was discovered by astronomer James Dunlop on May 7, 1826.NGC 5929
NGC 5929 is a Seyfert galaxy in the constellation Boötes. The pair of galaxies, NGC 5929 and NGC 5930, are interacting.NGC 7213
NGC 7213 is a lenticular galaxy located in the constellation Grus. It is located at a distance of circa 70 million light years from Earth, which, given its apparent dimensions, means that NGC 7213 is about 75,000 light years across. It was discovered by John Herschel on September 30, 1834. It is an active galaxy with characteristics between a type I Seyfert galaxy and LINER.PlanetPol
PlanetPol was a ground-based, high sensitivity polarimeter based at the William Herschel Telescope on the island of La Palma in the Canary Islands, Spain that has now been decommissioned. It was the most sensitive astronomical visual polarimeter ever built in fractional polarisation, a mantle that since its decommissioning now belongs to HIPPI. Although the device could be used for a wide range of astronomy, its primary use was the detection of extrasolar planets.Przybylski's Star
Przybylski's Star , or HD 101065, is a rapidly oscillating Ap star at roughly 355 light-years (109 parsecs) from the Sun in the southern constellation of Centaurus.QS Virginis
QS Virginis (abbreviated QS Vir) is an eclipsing binary system approximately 163 light-years away from the Sun, forming a cataclysmic variable. The system comprises an eclipsing white dwarf and red dwarf that orbit each other every 3.37 hours.V1494 Aquilae
V1494 Aquilae or NOVA Aquilae 1999 b was a nova which occurred in 1999 in the constellation Aquila and which reached a brightness of 4.0 mag.