The Koala: A Fast Blue Optical Transient with Luminous Radio Emission from a Starburst Dwarf Galaxy at z = 0.27

We present ZTF18abvkwla (the "Koala"), a fast blue optical transient discovered in the Zwicky Transient Facility (ZTF) One-Day Cadence (1DC) Survey. ZTF18abvkwla has a number of features in common with the groundbreaking transient AT 2018cow: blue colors at peak ( mag), a short rise time f...

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Veröffentlicht in:The Astrophysical journal 2020-05, Vol.895 (1), p.49
Hauptverfasser: Ho, Anna Y. Q., Perley, Daniel A., Kulkarni, S. R., Dong, Dillon Z. J., De, Kishalay, Chandra, Poonam, Andreoni, Igor, Bellm, Eric C., Burdge, Kevin B., Coughlin, Michael, Dekany, Richard, Feeney, Michael, Frederiks, Dmitry D., Fremling, Christoffer, Golkhou, V. Zach, Graham, Matthew J., Hale, David, Helou, George, Horesh, Assaf, Kasliwal, Mansi M., Laher, Russ R., Masci, Frank J., Miller, A. A., Porter, Michael, Ridnaia, Anna, Rusholme, Ben, Shupe, David L., Soumagnac, Maayane T., Svinkin, Dmitry S.
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Sprache:eng
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Zusammenfassung:We present ZTF18abvkwla (the "Koala"), a fast blue optical transient discovered in the Zwicky Transient Facility (ZTF) One-Day Cadence (1DC) Survey. ZTF18abvkwla has a number of features in common with the groundbreaking transient AT 2018cow: blue colors at peak ( mag), a short rise time from half-max of under two days, a decay time to half-max of only three days, a high optical luminosity ( mag), a hot ( 40,000 K) featureless spectrum at peak light, and a luminous radio counterpart. At late times ( ), the radio luminosity of ZTF18abvkwla ( at 10 , observer-frame) is most similar to that of long-duration gamma-ray bursts (GRBs). The host galaxy is a dwarf starburst galaxy ( , ) that is moderately metal-enriched ( ), similar to the hosts of GRBs and superluminous supernovae. As in AT2018cow, the radio and optical emission in ZTF18abvkwla likely arise from two separate components: the radio from fast-moving ejecta ( ) and the optical from shock-interaction with confined dense material (
ISSN:0004-637X
1538-4357
DOI:10.3847/1538-4357/ab8bcf