SN 2021gno: a calcium-rich transient with double-peaked light curves

Author:

Ertini K12ORCID,Folatelli G123,Martinez L124ORCID,Bersten M C123,Anderson J P56,Ashall C7,Baron E89,Bose S1011ORCID,Brown P J12,Burns C13,DerKacy J M87,Ferrari L12,Galbany L1415,Hsiao E16ORCID,Kumar S16,Lu J16,Mazzali P1718,Morrell N19,Orellana M420,Pessi P J1,Phillips M M19,Piro A L13,Polin A1321,Shahbandeh M16ORCID,Shappee B J22,Stritzinger M23,Suntzeff N B12,Tucker M22,Elias-Rosa N2414,Kuncarayakti H2526,Gutiérrez C P2526ORCID,Kozyreva A27ORCID,Müller-Bravo T E1415,Chen T -W28,Hinkle J T22ORCID,Payne A V22,Székely P2930,Szalai T293031ORCID,Barna B29ORCID,Könyves-Tóth R313233,Bánhidi D34,Bíró I B3034,Csányi I34,Kriskovits L3132,Pál A3132353637,Szabó Zs31323839,Szakáts R3132,Vida K3132,Vinkó J31323540,Gromadzki M41ORCID,Harvey L42ORCID,Nicholl M43ORCID,Paraskeva E44,Young D R45,Englert B46

Affiliation:

1. Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata , Paseo del Bosque S/N, B1900FWA La Plata, Argentina

2. Instituto de Astrofísica de La Plata (IALP), CCT-CONICET-UNLP , Paseo del Bosque S/N, B1900FWA La Plata, Argentina

3. Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo , 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583, Japan

4. Universidad Nacional de Río Negro. Sede Andina , Mitre 630, 8400 Bariloche, Argentina

5. European Southern Observatory , Alonso de Córdova 3107, Casilla 19, 8320000 Vitacura, Santiago, Chile

6. Millennium Institute of Astrophysics MAS , Nuncio Monsenor Sotero Sanz 100, Off. 104, 8320000 Providencia, Santiago, Chile

7. Department of Physics , Virginia Tech, Blacksburg, VA 24061, USA

8. Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma , 440 W. Brooks, Norman, OK 73019-2061, USA

9. Hamburger Sternwarte , Gojenbergsweg 112, D-21029 Hamburg, Germany

10. Department of Astronomy, The Ohio State University , 140 W. 18th Avenue, Columbus, OH 43210, USA

11. Center for Cosmology and AstroParticle Physics (CCAPP), The Ohio State University , 191 W. Woodruff Avenue, Columbus, OH 43210, USA

12. Mitchell Institute for Fundamental Physics and Astronomy, Department of Physics and Astronomy , Texas A&M University 4242 TAMU, College Station, TX 77845, USA

13. The Observatories of the Carnegie Institution for Science , 813 Santa Barbara St, Pasadena, CA 91101, USA

14. Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans , s/n, E-08193 Barcelona, Spain

15. Institut d’Estudis Espacials de Catalunya (IEEC) , E-08034 Barcelona, Spain

16. Department of Physics, Florida State University , 77 Chieftain Way, Tallahassee, FL 32306, USA

17. Astrophysics Research Institute, Liverpool John Moores University, IC2, Liverpool Science Park , 146 Brownlow Hill, Liverpool L3 5RF, UK

18. Max-Planck-Institut für Astrophysik , Karl-Schwarzschild Str 1, D-85748 Garching, Germany

19. Carnegie Observatories, Las Campanas Observatory , Casilla 601, 1700000 La Serena, Chile

20. Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET) ,C1425FQD Capital Federal, Argentina

21. TAPIR, Walter Burke Institute for Theoretical Physics , 350-17, Caltech, Pasadena, CA 91125, USA

22. Institute for Astronomy, University of Hawai‘i at Manoa , 2680 Woodlawn Dr, Honolulu, HI 96822, USA

23. Department of Physics and Astronomy, Aarhus University , Ny Munkegade 120, DK-8000 Aarhus C, Denmark

24. INAF – Osservatorio Astronomico di Padova , Vicolo dell’Osservatorio 5, I-35122 Padova, Italy

25. Tuorla Observatory, Department of Physics and Astronomy, University of Turku , FI-20014 Turku, Finland

26. Finnish Centre for Astronomy with ESO (FINCA), University of Turku , FI-20014 Turku, Finland

27. Heidelberger Institut f ür Theoretische Studien , Schloss-Wolfsbrunnenweg 35, D-69118 Heidelberg, Germany

28. The Oskar Klein Centre, Department of Astronomy, Stockholm University , AlbaNova, SE-10691 Stockholm, Sweden

29. Department of Experimental Physics, Institute of Physics, University of Szeged , Dóm tér 9, H-6720 Szeged, Hungary

30. ELKH-SZTE Stellar Astrophysics Research Group , Szegedi út, Kt. 766, H-6500 Baja, Hungary

31. Konkoly Observatory, Research Centre for Astronomy and Earth Sciences , Konkoly Thege Miklós út 15-17, H-1121 Budapest, Hungary

32. CSFK, MTA Centre of Excellence, Konkoly Thege Miklós út 15-17, H-1121 Budapest, Hungary

33. Gothard Astrophysical Observatory, ELTE Eötvös Loránd University , H-9400 Szombathely, Hungary

34. Baja Astronomical Observatory of University of Szeged , Szegedi út, Kt. 766, H-6500 Baja, Hungary

35. Eötvös Loránd University, Department of Astronomy , Pázmány Péter sétány 1/A, H-1117 Budapest, Hungary

36. Institute of Physics, Eötvös Loránd University , Pázmány Péter sétány 1/A, H-1117 Budapest, Hungary

37. MIT Kavli Institute for Astrophysics and Space Research , 70 Vassar Street, Cambridge, MA 02109, USA

38. Max-Planck-Institut für Radioastronomie , Auf dem Hügel 69, D-53121 Bonn, Germany

39. Scottish Universities Physics Alliance (SUPA), School of Physics and Astronomy, University of St Andrews, North Haugh , St Andrews KY16 9SS, UK

40. Department of Optics & Quantum Electronics, Institute of Physics, University of Szeged , Dóm tér 9, H-6720 Szeged, Hungary

41. Astronomical Observatory, University of Warsaw , Al. Ujazdowskie 4, PL-00-478 Warszawa, Poland

42. School of Physics, Trinity College Dublin, The University of Dublin , Dublin 2, Ireland

43. Birmingham Institute for Gravitational Wave Astronomy and School of Physics and Astronomy, University of Birmingham , Birmingham B15 2TT, UK

44. Department of Physics and Astronomy, University of California , Davis, One Shields Avenue, CA 95616, USA

45. Astrophysics Research Centre, School of Mathematics and Physics, Queen’s University Belfast , Belfast BT7 1NN, UK

46. Combate de los Pozos 1028 , C1222AAL Ciudad Autónoma de Buenos Aires, Argentina

Abstract

ABSTRACT We present extensive ultraviolet (UV) and optical photometric and optical spectroscopic follow-up of supernova (SN) 2021gno by the ‘Precision Observations of Infant Supernova Explosions’ (POISE) project, starting less than 2 d after the explosion. Given its intermediate luminosity, fast photometric evolution, and quick transition to the nebular phase with spectra dominated by [Ca ii] lines, SN 2021gno belongs to the small family of Calcium-rich transients. Moreover, it shows double-peaked light curves, a phenomenon shared with only four other Calcium-rich events. The projected distance from the centre of the host galaxy is not as large as other objects in this family. The initial optical light-curve peaks coincide with a very quick decline of the UV flux, indicating a fast initial cooling phase. Through hydrodynamical modelling of the bolometric light curve and line velocity evolution, we found that the observations are compatible with the explosion of a highly stripped massive star with an ejecta mass of $0.8\, M_\odot$ and a 56Ni mass of 0.024 M⊙. The initial cooling phase (first light-curve peak) is explained by the presence of an extended circumstellar material comprising ∼$10^{-2}\, {\rm M}_{\odot }$ with an extension of $1100\, R_{\odot }$. We discuss if hydrogen features are present in both maximum-light and nebular spectra, and their implications in terms of the proposed progenitor scenarios for Calcium-rich transients.

Funder

ANID

UNRN

NASA

European Social Fund

MCIN

AEI

CSIC

NSF

Independent Research Fund Denmark

Villum Fonden

MIUR

MICINN

FEDER

Horizon 2020 Framework Programme

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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