The MUSE view of the host galaxy of GRB 100316D

被引：28

作者：

Izzo, L. ^{[1
]}

Thone, C. C. ^{[1
]}

Schulze, S. ^{[2
,3
,4
,5
]}

Mehner, A. ^{[6
]}

Flores, H. ^{[7
]}

Cano, Z. ^{[1
]}

de Ugarte Postigo, A. ^{[1
,8
]}

Kann, D. A. ^{[1
]}

Amorin, R. ^{[9
,10
]}

Anderson, J. P. ^{[6
]}

Bauer, F. E. ^{[3
,4
,5
,11
]}

Bensch, K. ^{[1
]}

Christensen, L. ^{[8
]}

Covino, S. ^{[12
]}

Della Valle, M. ^{[13
]}

Fynbo, J. P. U. ^{[8
]}

Jakobsson, P. ^{[14
]}

Klose, S. ^{[15
]}

Kuncarayakti, H. ^{[16
,17
]}

Leloudas, G. ^{[2
]}

Milvang-Jensen, B. ^{[8
]}

Moller, P. ^{[18
]}

Puech, M. ^{[7
]}

Rossi, A. ^{[19
]}

Sanchez-Ramirez, R. ^{[1
]}

Vergani, S. D. ^{[7
]}

机构：

[1] CSIC, Inst Astrofis Andalucia, Glorieta Astron S-N, E-18008 Granada, Spain

[2] Weizmann Inst Sci, Dept Particle Phys & Astrophys, IL-7610001 Rehovot, Israel

[3] Pontificia Univ Catolica Chile, Inst Astrofis, Casilla 306, Santiago 22, Chile

[4] Pontificia Univ Catolica Chile, Ctr Astroingn, Casilla 306, Santiago 22, Chile

[5] Millennium Inst Astrophys MAS, Nuncio Monsenor Sotero Sanz 100, 7500011 Santiago, Chile

[6] European Southern Observ, Alonso de Cordova 3107,Casilla 19, Santiago 19001, Chile

[7] Univ Paris Diderot, PSL Res Univ, Observ Paris, GEPI,CNRS, 5 Pl Jules Janssen, F-92195 Meudon, France

[8] Univ Copenhagen, Niels Bohr Inst, Dark Cosmol Ctr, Juliane Maries Vej 30, DK-2100 Copenhagen, Denmark

[9] Univ Cambridge, Cavendish Lab, 19 JJ Thomson Ave, Cambridge CB3 0HE, England

[10] Univ Cambridge, Kavli Inst Cosmol, Madingley Rd, Cambridge CB3 0HA, England

[11] Space Sci Inst, 4750 Walnut St,Suite 205, Boulder, CO 80301 USA

[12] Osserv Astron Brera, Via Bianchi 46, I-23807 Merate, LC, Italy

[13] INAF, Osservatorio Astron Capodimonte, Salita Moiariello 16, I-80131 Naples, Italy

[14] Univ Iceland, Ctr Astrophys & Cosmol, Sci Inst, Dunhagi 5, IS-107 Reykjavik, Iceland

[15] Thuringer Landessternwarte Tautenburg, Sternwarte 5, D-07778 Tautenburg, Germany

[16] Univ Turku, Finnish Ctr Astron ESO FINCA, Vaisalantie 20, FI-21500 Pukkio, Finland

[17] Univ Turku, Dept Phys & Astron, Tuorla Observ, Vaisalantie 20, FI-21500 Pukkio, Finland

[18] European Southern Observ, Karl Schwarzschildstr 2, D-85748 Garching, Germany

[19] INAF IASF Bologna, CNR, Area Ric, Via Gobetti 101, I-40129 Bologna, Italy

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2017年 / 472卷 / 04期

关键词：

gamma-ray burst: general; gamma-ray burst: individual: GRB 100316D; galaxies: abundances; galaxies: general; galaxies: star formation; GAMMA-RAY BURSTS; CORE-COLLAPSE SUPERNOVAE; CHEMICAL ABUNDANCES; LUMINOSITY FUNCTION; MASS-DISTRIBUTION; ROTATION CURVES; LOW METALLICITY; LONG; EMISSION; STARBURST;

D O I：

10.1093/mnras/stx2244

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The low distance, z = 0.0591, of GRB 100316D and its association with SN 2010bh represent two important motivations for studying this host galaxy and the GRB's immediate environment with the integral field spectrographs like Very Large Telescope/Multi-Unit Spectroscopic Explorer. Its large field of view allows us to create 2D maps of gas metallicity, ionization level and the star formation rate (SFR) distribution maps, as well as to investigate the presence of possible host companions. The host is a late-type dwarf irregular galaxy with multiple star-forming regions and an extended central region with signatures of on-going shock interactions. The gamma-ray burst (GRB) site is characterized by the lowest metallicity, the highest SFR and the youngest (similar to 20-30 Myr) stellar population in the galaxy, which suggest a GRB progenitor stellar population with masses up to 20-40 M-circle dot. We note that the GRB site has an offset of similar to 660 pc from the most luminous SF region in the host. The observed SF activity in this galaxy may have been triggered by a relatively recent gravitational encounter between the host and a small undetected (L-H alpha <= 10(36) erg s(-1)) companion.

引用

页码：4480 / 4496

页数：17

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