Cover Picture: Astron. Nachr. 8/2024

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Main Authors: Hikmet Çakmak, Talar Yontan, Selçuk Bilir, Timothy S. Banks, Raúl Michel, Esin Soydugan, Seliz Koç, Hülya Erçay
Format: Artículo Open Access
Published: Wiley 2024
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author Hikmet Çakmak
Talar Yontan
Selçuk Bilir
Timothy S. Banks
Raúl Michel
Esin Soydugan
Seliz Koç
Hülya Erçay
author_facet Hikmet Çakmak
Talar Yontan
Selçuk Bilir
Timothy S. Banks
Raúl Michel
Esin Soydugan
Seliz Koç
Hülya Erçay
Hikmet Çakmak
Talar Yontan
Selçuk Bilir
Timothy S. Banks
Raúl Michel
Esin Soydugan
Seliz Koç
Hülya Erçay
collection Wiley Open Access
contents Cover Picture: Astron. Nachr. 8/2024 Hikmet Çakmak Talar Yontan Selçuk Bilir Timothy S. Banks Raúl Michel Esin Soydugan Seliz Koç Hülya Erçay Astronomische Nachrichten Vector‐Point Diagrams (left panels) and proper‐motion component vectors (right panels) for identified member stars in the open clusters Ruprecht 1 and Ruprecht 171. These two previously little‐studied open clusters, both at a distance of approximately 1.5 kpc, have been characterized and studied in some detail in the related paper by Çakmak and collaborators, published in this issue e240054.image 10.1002/asna.20249016 http://onlinelibrary.wiley.com/termsAndConditions#vor
doi_str_mv 10.1002/asna.20249016
format Artículo Open Access
id wiley_oa_10_1002_asna_20249016
institution Wiley Open Access
license_str_mv http://onlinelibrary.wiley.com/termsAndConditions#vor
publishDate 2024
publisher Wiley
record_format wiley_oa
spellingShingle Cover Picture: Astron. Nachr. 8/2024
Hikmet Çakmak
Talar Yontan
Selçuk Bilir
Timothy S. Banks
Raúl Michel
Esin Soydugan
Seliz Koç
Hülya Erçay
Astronomische Nachrichten
Cover Picture: Astron. Nachr. 8/2024 Hikmet Çakmak Talar Yontan Selçuk Bilir Timothy S. Banks Raúl Michel Esin Soydugan Seliz Koç Hülya Erçay Astronomische Nachrichten Vector‐Point Diagrams (left panels) and proper‐motion component vectors (right panels) for identified member stars in the open clusters Ruprecht 1 and Ruprecht 171. These two previously little‐studied open clusters, both at a distance of approximately 1.5 kpc, have been characterized and studied in some detail in the related paper by Çakmak and collaborators, published in this issue e240054.image 10.1002/asna.20249016 http://onlinelibrary.wiley.com/termsAndConditions#vor
title Cover Picture: Astron. Nachr. 8/2024
topic Astronomische Nachrichten
url https://onlinelibrary.wiley.com/doi/10.1002/asna.20249016