Proceedings of the International Astronomical Union
Overview
Proceedings of the International Astronomical Union is a scientific journal, published by Cambridge University Press since 2004 in English. The journal's country of origin is United Kingdom.
Details
Details
Abbr.
Proc Int Astron Union
Publisher
Cambridge University Press
Start
2004
End
Continuing
Frequency
Eight issues yearly
p-ISSN
1743-9213
e-ISSN
1743-9221
Country
United Kingdom
Language
English
Metrics
Metrics
h-index / Ranks: 11346
25
SJR / Ranks: 15090
121
CiteScore / Ranks: 15065
0.10
Recent Articles
1.
Fonfria J, Fernandez-Lopez M, Pardo J, Agundez M, Sanchez Contreras C, Velilla-Prieto L, et al.
Proc Int Astron Union
. 2025 Mar;
14(Suppl 343):398-399.
PMID: 40046511
AGB stars are important contributors of processed matter to the ISM. However, the physical and chemical mechanisms involved in its ejection are still poorly known. This process is expected to...
2.
Skowron D
Proc Int Astron Union
. 2024 Feb;
18(Suppl 376):180-194.
PMID: 38404362
Disentangling the structural components of the Milky Way requires knowledge of distances to various classes of objects, both young, which trace the Galactic disk, and old, which trace the Galactic...
3.
Quintana-Lacaci G, Velilla L, Fonfria J, Cernicharo J, Castro-Carrizo A, Agundez M, et al.
Proc Int Astron Union
. 2023 Dec;
669.
PMID: 38125701
Red Supergiant stars (RSGs) are known to eject large amounts of material during this evolutionary phase. However, the processes powering the mass ejection in low- and intermediate-mass stars do not...
4.
Miller A, Cioni M, de Grijs R, Sun N
Proc Int Astron Union
. 2023 Jun;
17(Suppl 373):11-14.
PMID: 37324748
The VISTA Magellanic Clouds Survey (VMC) is a near-infrared survey of the Magellanic system. The VMC data has been exploited to detect and study statistically correlated young groups of stars...
5.
Lanthermann C
Proc Int Astron Union
. 2023 Mar;
672:A6.
PMID: 36974081
The study of the multiplicity of massive stars gives hints of their formation processes and their evolution path. Optical interferometry is mandatory to fulfill our knowledge of their multiplicity by...
6.
El Mellah I, Cerutti B, Crinquand B, Parfrey K
Proc Int Astron Union
. 2023 Mar;
16(Suppl 362):184-189.
PMID: 36923908
The hot accretion flow around Kerr black holes is strongly magnetized. Magnetic field loops sustained by a surrounding accretion disk can close within the event horizon. We performed particle-in-cell simulations...
7.
Malhotra R
Proc Int Astron Union
. 2022 Jun;
15(Suppl 364):85-101.
PMID: 35651635
Perturbative analyses of planetary resonances commonly predict singularities and/or divergences of resonance widths at very low and very high eccentricities. We have recently reexamined the nature of these divergences using...
8.
Dwarkadas V
Proc Int Astron Union
. 2022 Jan;
14(Suppl 346):83-87.
PMID: 35096123
Massive stars lose a considerable amount of mass during their lifetime. When the star explodes as a supernova (SN), the resulting shock wave expands in the medium created by the...
9.
Pantazidis G, Scheffler M, Simonsen F, Cassidy A, Jensen P, Hornekaer L, et al.
Proc Int Astron Union
. 2021 Mar;
15(Suppl 350):458-459.
PMID: 33786061
Reactions on carbonaceous surfaces play an important role in processes such as H formation in the interstellar medium. We have investigated the adsorption of C molecules on a highly oriented...
10.
Young P
Proc Int Astron Union
. 2020 Dec;
15(Suppl 350):333-340.
PMID: 33294002
The Sun's atmosphere increases in temperature from 6000 degrees at the surface to over a million degrees at heights of a few thousand kilometers. This surprising temperature increase is still...