SN 2020faa , the SIMBAD biblio

SN 2020faa , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2022.08.19CEST18:43:53


Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
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
2021A&A...646A..22Y viz 187 T K A D     X C       3 5 ~ Is supernova
SN 2020faa an iPTF14hls look-alike?
YANG S., SOLLERMAN J., CHEN T.-W., et al.
2021MNRAS.504.5967S 47           X         1 3 ~ Double common envelope jets supernovae (CEJSNe) by triple-star systems. SOKER N.
2021MNRAS.506.2445S 47           X         1 5 ~ Binary neutron star merger in common envelope jets supernovae. SOKER N.
2021MNRAS.507.1651G 47           X         1 3 ~ Common envelope jets supernovae with a black hole companion as possible high-energy neutrino sources. GRICHENER A. and SOKER N.
2021MNRAS.508.2386S 47           X         1 6 ~ Simulating highly eccentric common envelope jet supernova impostors. SCHREIER R., HILLEL S., SHIBER S., et al.
2022MNRAS.509.2836S 50           X         1 3 ~ Spin-orbit misalignment from triple-star common envelope evolution. SOKER N.
2022ApJ...926L..11S 50           X         1 51 ~ Optical Rebrightening of Extragalactic Transients from the Zwicky Transient Facility. SORAISAM M., MATHESON T., LEE C.-H., et al.
2022ApJ...927..148C 50           X         1 3 ~ A Physical Model of Delayed Rebrightenings in Shock-interacting Supernovae without Narrow-line Emission. COUGHLIN E.R. and ZRAKE J.
2022RAA....22e5010S 50           X         1 14 ~ A Common Envelope Jets Supernova (CEJSN) Impostor Scenario for Fast Blue Optical Transients. SOKER N.
2022ApJ...933..102W 50           X         1 4 ~ iPTF14hls in the Circumstellar Medium Interaction Model: A Promising Candidate for a Pulsational Pair-instability Supernova. WANG L.-J., LIU L.-D., LIN W.-L., et al.

goto View the references in ADS


2022.08.19-18:43:53

© Université de Strasbourg/CNRS

    • Contact