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Ata uhi

I tiakina i:
Ngā taipitopito rārangi puna kōrero
Ngā kaituhi matua: Wielgórski, Piotr, Pietrzyński, Grzegorz, Gieren, Wolfgang, Zgirski, Bartlomiej, Narloch, Weronika, Hajdu, Gergely, Storm, Jesper, Nardetto, Nicolas, Kervella, Pierre, Pilecki, Bogumił, Górski, Marek, Smolec, Radosław, Salinas, Ricardo, Graczyk, Dariusz, Hocdé, Vincent, Karczmarek, Paulina, Taormina, Monica, Pych, Wojciech, Netzel, Henryka, Chini, Rolf, Hodapp, Klaus, Kałuszyński, Mikołaj, Nuñez, Francisco Pozo, Kotysz, Krzysztof, Moździerski, Dawid, Mikołajczyk, Przemysław, Kołaczek-Szymański, Piotr
Hōputu: Preprint
I whakaputaina: 2026
Ngā marau:
Solar and Stellar Astrophysics
Astrophysics of Galaxies
Urunga tuihono:https://arxiv.org/abs/2603.28472
Ngā Tūtohu: Tāpirihia he Tūtohu
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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Ngā tūemi rite

  • Projection factor and radii of Type II Cepheids
    mā: Wielgórski, Piotr, me ētahi atu.
    I whakaputaina: (2024)
  • Period-Luminosity Relations for Galactic Type II Cepheids in the Sloan bands
    mā: Narloch, W., me ētahi atu.
    I whakaputaina: (2025)
  • Period-luminosity and period-luminosity-metallicity relations for Galactic RR Lyrae stars in the Sloan bands
    mā: Narloch, W., me ētahi atu.
    I whakaputaina: (2024)
  • Cepheids with giant companions. II. Spectroscopic confirmation of nine new double-lined binary systems composed of two Cepheids
    mā: Pilecki, Bogumił, me ētahi atu.
    I whakaputaina: (2024)
  • Distance to the Globular Cluster M 3 from the Infrared Surface Brightness Technique applied to RR Lyrae stars
    mā: Zgirski, Bartłomiej, me ētahi atu.
    I whakaputaina: (2025)

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