420 citations
- Center for Astrophysics Harvard & SmithsonianUS73 papers
- Konkoly ObservatoryHU50 papers
- Princeton UniversityUS49 papers
- University of California, BerkeleyUS42 papers
- Australian National UniversityAU30 papers
- University of CopenhagenDK30 papers
- Max Planck Institute for AstronomyDE29 papers
- Pontificia Universidad Católica de ChileCL29 papers
- California Institute of TechnologyUS25 papers
- Kyoto UniversityJP22 papers
- Millennium Institute of AstrophysicsCL22 papers
- Crimean Astrophysical ObservatoryUA20 papers
103 papers
GOTO065054+593624: a 8.5 mag amplitude dwarf nova identified in real time via Kilonova Seekers
T. L. Killestein, G. Ramsay, M. Kennedy +62
Dwarf novae are astrophysical laboratories for probing the nature of accretion, binary mass transfer, and binary evolution -- yet their diverse observational characteristics contin…
2021 superoutburst of WZ Sge-type dwarf nova V627 Pegasi lacks an early superhump phase
Yusuke Tampo, Taichi Kato, Naoto Kojiguchi +27
Superoutbursts in WZ Sge-type dwarf novae (DNe) are characterized by both early superhumps and ordinary superhumps originating from the 2:1 and 3:1 resonances, respectively. Howeve…
PNV J00444033+4113068: early superhumps with 0.7 mag amplitude and non-red color
Yusuke Tampo, Keisuke Isogai, Naoto Kojiguchi +13
In the first days of WZ Sge-type dwarf nova (DN) outbursts, the 2:1 resonance induces a spiral arm structure in the accretion disk, which is observed as early superhumps in optical…
Review of synergic meteor observations: linking the results from cameras, ionosondes, infrasound and seismic detectors
Á. Kereszturi, V. Barta, I. Bondár +6
Joint evaluation of different meteor observation types support the better understanding of both the meteor phenomenon and the terrestrial atmosphere. Two types of examples are pres…
The Fast Evolving, Tremendous and Blue Superoutburst in ASASSN-21au Reveals a Dichotomy in the Outbursts of Long-period AM CVns
L. E. Rivera Sandoval, C. O. Heinke, J. M. Hameury +4
ASASSN-21au is an ultracompact accreting white dwarf binary (AM CVn) with a period of approx. 58 min. Using multiwavelength observations of the system, we discovered a dichotomy in…
On the nature of the anomalous event in 2021 in the dwarf nova SS Cygni and its multi-wavelength transition
Mariko Kimura, Shinya Yamada, Nozomi Nakaniwa +20
SS Cyg has long been recognized as the prototype of a group of dwarf novae that show only outbursts. However, this object has entered a quite anomalous event in 2021, which at firs…