Discipline | Astronomy, Astrophysics |
---|---|
Language | English |
Edited by | Thierry Forveille, João Alves |
Publication details | |
History | 1969–present |
Publisher | EDP Sciences on behalf of the European Southern Observatory |
Frequency | Monthly |
Yes | |
License | CC BY 4.0 |
6.5 (2022) | |
Standard abbreviations | |
ISO 4 | Astron. Astrophys. |
Indexing | |
CODEN | AAEJAF |
ISSN | 0004-6361 (print) 1432-0746 (web) |
LCCN | 74220573 |
OCLC no. | 1518497 |
Links | |
Astronomy & Astrophysics (A&A) [1] is a monthly peer-reviewed scientific journal covering theoretical, observational, and instrumental astronomy and astrophysics. It is operated by an editorial team under the supervision of a board of directors representing 27 sponsoring countries plus a representative of the European Southern Observatory. The journal is published by EDP Sciences and the current editors-in-chief are Thierry Forveille and João Alves.
Astronomy & Astrophysics was created as an answer to the publishing situation found in Europe in the 1960s. At that time, multiple journals were being published in several countries around the continent. These journals usually had a limited number of subscribers, and articles were written in languages other than English. They were less widely read than American and British journals and the research they reported had therefore less impact in the community. [2]
Starting in 1963, conversations between astronomers from European countries assessed the need for a common astronomical journal. On 8 April 1968, leading astronomers from Belgium, Denmark, France, Germany, the Netherlands, and Scandinavian countries met in Leiden University to prepare a possible merging of some of the principal existing journals. It was proposed that the new journal be called Astronomy and Astrophysics, A European Journal. [3]
The main policy-making body of the new journal was to be the "Board of Directors", consisting of senior astronomers or government representatives of the sponsoring countries. The board appoints the editors-in chief, who are responsible for the scientific contents of the journal. The European Southern Observatory was chosen as an additional body that acts on behalf of the board and handles the administrative, financial, and legal matters of the journal.
A second meeting held in July 1968 in Brussels cemented the agreement discussed in Leiden. Each nation established an annual monetary contribution and appointed its delegates for the board of directors. Also at this meeting, the first editors-in-chief were appointed: Stuart Pottasch and Jean-Louis Steinberg.
The next meeting took place in Paris on 11 October 1968 and is officially regarded as the first meeting of the board of directors. At this meeting, the first chairman of the board, Adriaan Blaauw, was appointed, and the contract with the publisher Springer Science+Business Media was formalized.
The first issue of A&A was published in January 1969, merging several national journals of individual European countries into one comprehensive publication. [2] [3] [4] These journals, with their ISSN and date of first publication, are as follows:
Arkiv för Astronomi ( ISSN 0004-2048), established in 1948 in Sweden, was also incorporated in 1973. The publishing of Astronomy & Astrophysics was further extended in 1992 by the incorporation of Bulletin of the Astronomical Institutes of Czechoslovakia (ISSN 0004-6248), established in 1947.
There were only four issues of the journal in 1969, but it soon became a monthly publication and one of the four major generalist astronomical journals in the world. Initially, papers were submitted in English, French or German, but it soon became clear that, for a given author, the papers in English were cited twice as often as those in other languages.
In addition to regular research papers in several different fields of astrophysics. A&A featured Letters and Research Notes for short manuscripts on a significant result or idea. A Supplement Series for the journal was created in 1970 for publishing extensive tabular material and catalogs.
The turn of the century brought important changes to the journal. In 2001, a new contract was signed with EDP Sciences, which replaced Springer as the publishing house. Special Issues featuring results of astronomical surveys and space missions such as XMM-Newton, Planck, Rosetta, and Gaia were introduced.
The editorial structure of the journal was profoundly changed in 2003 [5] and 2005 [6] to involve more countries in the editorial process and to better handle the increasing number of submissions. Precise criteria for publishing in Astronomy & Astrophysics were explicited in 2004. [7] English language editing was introduced in 2001 as a service to the diverse authorship of the journal. [8] An extensive survey of authors conducted in 2007 [9] showed widespread satisfaction with the new directions of the journal, although the use of structured abstracts [10] proved more controversial.
The evolution of electronic publishing resulted in the extinction of the Supplement Series, which was incorporated in the main journal in 2001, and of the printed edition in 2016. [11] The Research Notes section was also discontinued in 2016. [12]
In 2023, A&A announced the introduction of links between articles and corresponding ESO datasets.
The journal editorial office is located at the Paris Observatory and is supervised by the managing editor. It handles over 2000 papers per year.
An archive of the published articles and related material is maintained by the Centre de données astronomiques de Strasbourg.
The original sponsoring countries were the four countries whose journals merged to form Astronomy & Astrophysics (France, Germany, the Netherlands and Sweden), together with Belgium, Denmark, Finland, and Norway. Norway later withdrew, but Austria, Greece, Italy, Spain, and Switzerland joined during the 1970s and 1980s. The Czech Republic, Estonia, Hungary, Poland, and Slovakia all joined as new members in the 1990s.
In 2001 the words "A European Journal" were removed from the front cover in recognition of the fact that the journal was becoming increasingly global in scope. In effect, Argentina was admitted as an "observer" in 2002. In 2004 the board of directors decided that the journal "will henceforth consider applications for sponsoring membership from any country in the world with well-documented active and excellent astronomical research". [13] Argentina became the first non-European country to gain full membership in 2005, followed by Brazil and Chile in 2006 (Brazil withdrew in 2016). Other European countries also joined during the 21st century: Portugal, Croatia, and Bulgaria during the 2010s, and Armenia, Lithuania, Norway, Serbia and Ukraine in the 2010s.The current list of member countries is listed here. [14]
The following persons are or have been chairs of the Board of Directors:
Before 2022, the most recent issue of A&A was available free of charge for readers. Authors had the option to pay article processing charges (APC) for immediate and permanent open access. Furthermore, all Letters to the Editor and all articles published in Sections 12 to 15 were in free access at no cost to the authors. Articles in the other sections of the journal were made freely available 12 months after publication (delayed open-access), through the publisher's site and via the Astrophysics Data System.
Since the beginning of 2022, Astronomy & Astrophysics is published in full open access under the Subscribe to Open (S2O) model.
A&A organises Scientific Writing Schools [15] aimed at postgraduate students and young researchers. The purpose of these schools is to teach young authors how to express their scientific results through adequate and efficient science writing. As of 2019, five of these schools were organised in Belgium (2008 and 2009), Hungary (2014), Chile (2016) and China (2019).
This journal is abstracted and indexed in:
According to the Journal Citation Reports , the journal has a 2022 impact factor of 6.5. [23]
Tau Boötis, Latinised from τ Boötis, is an F-type main-sequence star approximately 51 light-years away in the constellation of Boötes. It is a binary star system, with the secondary star being a red dwarf. In 1999, an extrasolar planet was detected orbiting the primary star.
HD 142 is a wide binary star system in the southern constellation of Phoenix. The main component has a yellow-white hue and is dimly visible to the naked eye with an apparent visual magnitude of 5.7. The system is located at a distance of 85.5 light years from the Sun based on parallax measurements, and is drifting further away with a radial velocity of +6 km/s.
N Centauri is a binary star in the southern constellation of Centaurus. The brighter star is dimly visible to the naked eye with an apparent visual magnitude of 5.26, and it is approximately 304 light years away based on parallax. It has an absolute magnitude of +0.76 and is drifting further away from the Sun with a radial velocity of +27 km/s. It is a candidate member of the Sco OB2 moving group.
The Dark Doodad Nebula is a dark nebula near the globular cluster NGC 4372, much closer than the centre of the galaxy and in the galactic plane, having a length of nearly three degrees of arc. Although officially unnamed, this long molecular cloud has come to be known under this name. It can be found in the southern constellation of Musca with strong binoculars.
HD 24479, also designated as HR 1204, is a solitary, bluish-white hued star located in the northern circumpolar constellation Camelopardalis. The star is visible to the naked eye with an apparent visual magnitude of 5.04. Based on Gaia DR3 parallax measurements, it is located 385 light years from the Sun. However, it is receding with a somewhat constrained heliocentric radial velocity of 4.6 km/s. At its current distance, HD 24479's brightness is diminished by 0.29 magnitudes due to interstellar dust.
Georges Meylan is a Swiss astronomer, born on July 31, 1950, in Lausanne, Switzerland. He was the director of the Laboratory of Astrophysics of the Swiss Federal Institute of Technology (EPFL) in Lausanne, Switzerland, and now a professor emeritus of astrophysics and cosmology at EPFL. He is still active in both research and teaching.
DS Tucanae is a binary star system 144 light years away in the constellation of Tucana. It has an apparent visual magnitude of 8.5, and is a RS Canum Venaticorum variable. The system is notable for being young as a member of the 45 Myr old Tucana-Horologium moving group and for the primary star hosting the confirmed exoplanet DS Tucanae Ab, discovered by THYME, using TESS.
HD 26764, also known as HR 1314 or rarely 14 H. Camelopardalis, is a solitary white hued star located in the northern circumpolar constellation Camelopardalis. It has an apparent magnitude of 5.19, making it faintly to the naked eye if viewed under good conditions. Gaia DR3 parallax measurements place the object at a distance of 266 light years and is drifting closer with a poorly constrained heliocentric radial velocity of 3 km/s. At its current distance, HD 26764's brightness is diminished by 0.26 magnitudes due to interstellar dust.
HD 212771, also named Lionrock, is a solitary star in the southern zodiac constellation Aquarius. It has an apparent magnitude of 7.60, making it readily visible with binoculars but not the naked eye. Parallax measurements place the object at a distance of 364 light years, and is currently receding with a radial velocity of 15 km/s.
10 Trianguli, or simply 10 Tri is a solitary star located in the northern constellation Triangulum. It is faintly visible to the naked eye as a white-hued point of light with an apparent magnitude of 5.29. Gaia DR3 parallax measurements imply a distance of 363 light-years and it is slowly receding with a heliocentric radial velocity of 0.4 km/s. At its current distance, 10 Tri's brightness is diminished by an interstellar extinction of 0.11 magnitudes and it has an absolute magnitude of −0.02.
HD 33519, also known as HR 1682, is a probable spectroscopic binary located in the southern circumpolar constellation Mensa. It is one of the stars near the limit of naked eye visibility, having an apparent magnitude of 6.28. The system is relatively far at a distance of 940 light years but is approaching with a heliocentric radial velocity of −2.5 km/s. However, this value is poorly constrained.
CW Octantis, also known as HD 148542, is a solitary, white hued variable star located in the southern circumpolar constellation Octans. It has an apparent magnitude of 6.03, allowing it to be faintly visible to the naked eye. Parallax measurements from Gaia DR3 place the object at a distance of 629 light years. It appears to be receding from the Solar System with a heliocentric radial velocity of 7.1 km/s.
40 Leonis Minoris is a white hued star located in the northern constellation Leo Minor. It is rarely called 14 H. Leonis Minoris, which is the designation given by Polis astronomer Johann Hevelius.