ASASSN -14ho , the SIMBAD biblio

ASASSN -14ho , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST10:29:22

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2014ATel.6619....1P 193 T         X         4 2 ~ The outburst of the bright CV
ASASSN-14ho. 		PRIETO J.L., STURCH L., MADORE B., et al.
2019AJ....158..156G 1015 T   A D S   X C       23 4 ~ Two long-period cataclysmic variable stars:
ASASSN-14ho and V1062 Cyg. 		GASQUE L.C., HENING C.A., HVIDING R.E., et al.
2020PASJ...72L...2K 477 T   A     X C       10 5 ~
ASASSN-14ho: Longest-period dwarf nova with multiple rebrightenings. 		KATO T.
2020PASJ...72...14K 41           X         1 111 14 Survey of period variations of superhumps in SU UMa-type dwarf novae. X. The tenth year (2017). KATO T., ISOGAI K., WAKAMATSU Y., 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 84           X         2 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 184       D     X         5 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 42           X         1 6 ~ BO Ceti: Dwarf nova showing both IW And-type and SU UMa-Type features. KATO T., TAMPO Y., KOJIGUCHI N., et al.
2021PASJ...73.1375K 42           X         1 13 ~ New candidates for AM Canum Venaticorum stars among ASAS-SN transients. KATO T. and KOJIGUCHI N.
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.

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