Long-period Variables
Long-Period Variables is a class of pulsating variable stars characterized by orbital periods exceeding 100 days, distinguished from other variable star types by their extended periodicity and association with late spectral types undergoing radial pulsations in the asymptotic giant branch phase.
359
Publications
15.4K
Citations
918
Authors
361
Institutions
Publications per year
2017–2026
36
Variants
Lpvs
Parents
359
P. R. Wood, M. S. Bessell, M. W. Fox · The Astrophysical Journal · 1983 · 304 citations · Full text
Natural Sciences, Astronomy, Physics +12
The Distance to NGC 5128 (Centaurus A)
Publications of the Astronomical Society of Australia · 2010 · 224 citations · Full text
Natural Sciences, Astronomy, Physics +15
1–5 of 359
918
22
h-index
13
h-index
9
h-index
8
h-index
7
h-index
1–5 of 918
361

Centre National de la Recherche Scientifique
Paris, France
20 h-index
37 publications
1.8K citations

Mount Stromlo Observatory
Canberra, Australia
18 h-index
29 publications
1.7K citations

Australian National University
Canberra, Australia
17 h-index
24 publications
1.1K citations
South African Radio Astronomy Observatory
Cape Town, South Africa
16 h-index
33 publications
1.5K citations
University of Vienna
Vienna, Austria
14 h-index
28 publications
1.3K citations
Osservatorio Astronomico di Padova
Padua, Italy
13 h-index
41 publications
1.6K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
13 h-index
20 publications
726 citations
Institut d'Astrophysique de Paris
Paris, France
12 h-index
22 publications
1.1K citations
1–8 of 361
ApJ · 106 publications · 4.5K citations
37
h-index
68 publications · 2.9K citations
30
h-index
AJ · 45 publications · 2.1K citations
29
h-index
46 publications · 1.9K citations
26
h-index
13 publications · 744 citations
13
h-index
1–5