Recovering Lost Light: Discovery of Supernova Remnants with Integral Field Spectroscopy


Por: Martínez-Rodríguez, H, Galbany, L, Badenes, C, Anderson, JP, Domínguez, I, Kuncarayakti, H, Lyman, JD, Sánchez, SF, Vílchez, JM, Smith, N, Milisavljevic, D

Publicada: 1 mar 2024
Resumen:
We present results from a systematic search for broad (>= 400 km s-1) H alpha emission in integral field spectroscopy data cubes of similar to 1200 nearby galaxies obtained with PMAS and MUSE. We found 19 unique regions that pass our quality cuts, four of which match the locations of previously discovered supernovae (SNe): one Type IIP and three Type IIn, including the well-known SN 2005ip. We suggest that these objects are young Supernova remnants (SNRs), with bright and broad H alpha emission powered by the interaction between the SN ejecta and dense circumstellar material. The stellar ages measured at the locations of these SNR candidates are systematically lower by about 0.5 dex than those measured at the locations of core-collapse (CC) SNe, implying that their progenitors might be shorter lived and therefore more massive than a typical CCSN progenitor. The methods laid out in this work open a new window into the study of nearby SNe with integral field spectroscopy.

Filiaciones:
Martínez-Rodríguez, H:
 Univ Pittsburgh, Astrophys & Cosmol Ctr PITT PACC, Dept Phys & Astron, 3941 OHara St, Pittsburgh, PA 15260 USA

 Univ Pittsburgh, Astrophys & Cosmol Ctr PITT PACC, Pittsburgh Particle Phys, 3941 OHara St, Pittsburgh, PA 15260 USA

Galbany, L:
 CSIC, Inst Space Sci ICE, Campus UAB,Carrer Can Magrans S-N, E-08193 Barcelona, Spain

 Inst Estudis Espacials Catalunya IEEC, c Gran Capita 2-4, E-08034 Barcelona, Spain

Badenes, C:
 Univ Pittsburgh, Astrophys & Cosmol Ctr PITT PACC, Dept Phys & Astron, 3941 OHara St, Pittsburgh, PA 15260 USA

 Univ Pittsburgh, Astrophys & Cosmol Ctr PITT PACC, Pittsburgh Particle Phys, 3941 OHara St, Pittsburgh, PA 15260 USA

Anderson, JP:
 European Southern Observ, Alonso de Cordova 3107,Casilla 190001, Santiago, Chile

 Millennium Inst Astrophys MAS, Nuncio Monsenor Sotero Sanz 100,Off 104, Santiago, Chile

Domínguez, I:
 Univ Granada, Dept Fis Teor & Cosmos, E-18071 Granada, Spain

Kuncarayakti, H:
 Univ Turku, Dept Phys & Astron, Tuorla Observ, Vaisalantie 20, FI-21500 Piikkio, Finland

Lyman, JD:
 Univ Warwick, Dept Phys, Coventry CV4 7AL, England

Sánchez, SF:
 Univ Nacl Autoonoma Mexico, Inst Astron, AP 70-264, Mexico City 04510, DF, Mexico

Vílchez, JM:
 Inst Astrofis Andalucia CSIC, Glorieta Astron S-N, E-18008 Granada, Spain

Smith, N:
 Univ Arizona, Steward Observ, 933 N Cherry Aveue, Tucson, AZ 85721 USA

Milisavljevic, D:
 Purdue Univ, Dept Phys & Astron, W Lafayette, IN 47907 USA

 Purdue Univ, Integrat Data Sci Initiat, W Lafayette, IN 47907 USA
ISSN: 0004637X





ASTROPHYSICAL JOURNAL
Editorial
UNIV CHICAGO PRESS, 1427 E 60TH ST, CHICAGO, IL 60637-2954 USA, Estados Unidos America
Tipo de documento: Article
Volumen: 963 Número: 2
Páginas:
WOS Id: 001180030800001
imagen Green Accepted, gold