UCAC4 761-008050 , the SIMBAD biblio

UCAC4 761-008050 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST09:08:37


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Title First 3 Authors
2019PASJ...71L...1K 41           X         1 10 ~ Discovery of standstills in the SU UMa-type dwarf nova NY Serpentis. KATO T., PAVLENKO E.P., PIT N.V., et al.
2020MNRAS.494.5775H 16       D               1 120 ~ Cataclysmic variables as possible counterparts of ancient Far Eastern guest stars. HOFFMANN S.M. and VOGT N.
2021MNRAS.505.1135F viz 17       D               1 25035 ~ Population-based identification of H α-excess sources in the Gaia DR2 and IPHAS catalogues. FRATTA M., SCARINGI S., DREW J.E., et al.
2021MNRAS.505.2051E 126           X   F     2 13 18 LAMOST J0140355 + 392651: an evolved cataclysmic variable donor transitioning to become an extremely low-mass white dwarf. EL-BADRY K., QUATAERT E., RIX H.-W., et al.
2021MNRAS.508.4106E 42           X         1 65 22 Birth of the ELMs: a ZTF survey for evolved cataclysmic variables turning into extremely low-mass white dwarfs. EL-BADRY K., RIX H.-W., QUATAERT E., et al.
2021PASJ...73.1209W 1212 T K A D     X C       28 19 10
ASASSN-18aan: An eclipsing SU UMa-type cataclysmic variable with a 3.6-hr orbital period and a late G-type secondary star.
WAKAMATSU Y., THORSTENSEN J.R., KOJIGUCHI N., et al.
2021PASJ...73.1280K 84           X         2 6 ~ BO Ceti: Dwarf nova showing both IW And-type and SU UMa-Type features. KATO T., TAMPO Y., KOJIGUCHI N., et al.
2023AJ....165..163C viz 17       D               1 1619 ~ Galactic Model Parameters and Spatial Density of Cataclysmic Variables in the Gaia Era: New Constraints on Population Models. CANBAY R., BILIR S., OZDONMEZ A., et al.
2024A&A...691A.249S viz 18       D               2 107 ~ New orbital periods of high-inclination dwarf novae based on Gaia Alerts photometry. SAEZ-CARVAJAL C., VOGT N., ZOROTOVIC M., et al.
2025A&A...699A..81K viz 47         O X         1 17 ~ Hot donors in cataclysmic variables: The case of EI Psc. KARA J., ZHARIKOV S., WOLF M., et al.

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