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Astronomy & Astrophysics (A&A)

Publisher :

EDP Sciences

Scopus Profile
Peer reviewed only
Scopus Profile
Open Access
  • Astronomy
  • Astrophysics
  • Planetary Science

    • +1

e-ISSN :

1432-0746

Issue Frequency :

Monthly

Impact Factor :

6,240

p-ISSN :

0004-6361

Est. Year :

1980

Mobile :

33476514206

DOI :

YES

Country :

France

Language :

English

APC :

YES

Impact Factor Assignee :

Google Scholar

Email :

editorial.office@aanda.org

Journal Descriptions

Astronomy & Astrophysics (A&A) is a peer-reviewed journal that publishes original research in astronomy and astrophysics. The journal is an international consortium governed by a Board of Directors. The Board sets the policies for A&A including general guidelines for publishing, the selection of the Editors, the various financial aspects, as well as membership of new countries. The mission of A&A is: Publish important original work that stimulates high-quality scientific discourse Safeguard scientific reproducibility and ethical best practices Educate early-career astronomers on scientific writing A&A is a community journal. Publication decisions are in the sole hands of the Editors charged to implement a rigorous peer-reviewed process. The Editors are astronomers that are independent of any government or administrative body associated with the journal. Detailed publication policies, and research areas, are available on the journal web pages. A&A promotes diversity and equity in science. A&A embraces open, inclusive, and fair practices that reflect the culture and values of the worldwide community of astronomers.


Astronomy & Astrophysics (A&A) is :

International, Peer-Reviewed, Open Access, Refereed, Astronomy, Astrophysics, Planetary Science, Planetary Sciences , Online or Print, Monthly Journal

UGC Approved, ISSN Approved: P-ISSN - 0004-6361, E-ISSN - 1432-0746, Established in - 1980, Impact Factor - 6,240

Provide Crossref DOI

Indexed in Scopus, WoS, PubMed

Not indexed in DOAJ, UGC CARE

Indexing

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WoS
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+6 More

Publications of A&A

  • dott image October, 2016

The segregation of starless and protostellar clumps in the Hi-GAL ℓ = 224° region

Context. Stars form in dense, dusty structures, which are embedded in larger clumps of molecular clouds often showing a clear filamentary structure on large scales (≳1 pc). The origin (e.g...

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