[HTML][HTML] The evolutionary state of Miras with changing pulsation periods
Astronomy & Astrophysics, 2011 - aanda.org
Context. Miras are long-period variables thought to be in the asymptotic giant branch (AGB)
phase of evolution. In about one percent of known Miras, the pulsation period is changing. It …
phase of evolution. In about one percent of known Miras, the pulsation period is changing. It …
[PDF][PDF] The evolutionary state of Miras with changing pulsation periods
S Uttenthaler, K Van Stiphout, K Voet, H Van Winckel… - 2011 - academia.edu
Context. Miras are long-period variables thought to be in the asymptotic giant branch (AGB)
phase of evolution. In about one percent of known Miras, the pulsation period is changing. It …
phase of evolution. In about one percent of known Miras, the pulsation period is changing. It …
[PDF][PDF] The evolutionary state of Miras with changing pulsation periods
S Uttenthaler, K Van Stiphout, K Voet, H Van Winckel… - A&A, 2011 - scholar.archive.org
Context. Miras are long-period variables thought to be in the asymptotic giant branch (AGB)
phase of evolution. In about one percent of known Miras, the pulsation period is changing. It …
phase of evolution. In about one percent of known Miras, the pulsation period is changing. It …
The evolutionary state of Miras with changing pulsation periods
S Uttenthaler, K van Stiphout, K Voet… - Astronomy and …, 2011 - ui.adsabs.harvard.edu
Context. Miras are long-period variables thought to be in the asymptotic giant branch (AGB)
phase of evolution. In about one percent of known Miras, the pulsation period is changing. It …
phase of evolution. In about one percent of known Miras, the pulsation period is changing. It …
[引用][C] The evolutionary state of Miras with changing pulsation periods
S Uttenthaler, K Van Stiphout, K Voet… - Astronomy & …, 2011 - cir.nii.ac.jp
The evolutionary state of Miras with changing pulsation periods | CiNii Research CiNii 国立
情報学研究所 学術情報ナビゲータ[サイニィ] 詳細へ移動 検索フォームへ移動 論文・データをさがす …
情報学研究所 学術情報ナビゲータ[サイニィ] 詳細へ移動 検索フォームへ移動 論文・データをさがす …
[引用][C] The evolutionary state of Miras with changing pulsation periods
S UTTENTHALER, K VAN STIPHOUT… - Astronomy and …, 2011 - pascal-francis.inist.fr
Author UTTENTHALER, S 1 2; VAN STIPHOUT, K 1 3; WAELKENS, C 1; FREMAT, Y 5;
HENSBERGE, H 5; DUMORTIER, L 5; LEHMANN, H 6; VOET, K 1; VAN WINCKEL, H 1; …
HENSBERGE, H 5; DUMORTIER, L 5; LEHMANN, H 6; VOET, K 1; VAN WINCKEL, H 1; …
The evolutionary state of Miras with changing pulsation periods
S Uttenthaler, K Van Stiphout, K Voet… - arXiv preprint arXiv …, 2011 - arxiv.org
Context: Miras are long-period variables thought to be in the asymptotic giant branch (AGB)
phase of evolution. In about one percent of known Miras, the pulsation period is changing. It …
phase of evolution. In about one percent of known Miras, the pulsation period is changing. It …
[引用][C] The evolutionary state of Miras with changing pulsation periods
S Uttenthaler, K van Stiphout, K Voet… - Astronomy & …, 2011 - difusion.ulb.ac.be
[PDF][PDF] The evolutionary state of Miras with changing pulsation periods
S Uttenthaler, K Van Stiphout, K Voet, H Van Winckel… - A&A, 2011 - researchgate.net
Context. Miras are long-period variables thought to be in the asymptotic giant branch (AGB)
phase of evolution. In about one percent of known Miras, the pulsation period is changing. It …
phase of evolution. In about one percent of known Miras, the pulsation period is changing. It …
[引用][C] The evolutionary state of Miras with changing pulsation periods
S Uttenthaler, K van Stiphout, K Voet, H van Winckel… - orfeo.belnet.be
The evolutionary state of Miras with changing pulsation periods Toggle navigation Login Toggle
navigation View Item ORFEO Home Royal Observatory of Belgium and the Planetarium ROB …
navigation View Item ORFEO Home Royal Observatory of Belgium and the Planetarium ROB …