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Grb 980425 Host: [C Ii], [O I], and Co Lines Reveal Recent Enhancement of Star Formation Due to Atomic Gas Inflow

AuthID
P-00M-999

Author(s)

Michalowski, MJ

Castro Ceron, JMC

Wardlow, JL

Karska, A

Messias, H

van der Werf, P

Hunt, LK

Baes, M

Castro Tirado, AJ

Gentile, G

[+1]·

Le Floc'h, E

Perez Martinez, R

Guelbenzu, AN

Rasmussen, J

Rizzo, JR

Rossi, A

Sanchez Portal, M

Schady, P

Sollerman, J

Xu, D

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Tipo de Documento

Article

Year published

2016

Publicado

in ASTRONOMY & ASTROPHYSICS, ISSN: 1432-0746

Volume: 595

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Publication Identifiers

DOI: 10.1051/0004-6361/201629441

Wos: WOS:000388573500132

Source Identifiers

ISSN: 1432-0746

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All authors

Name Order	Nome	Name Order	Nome	Name Order	Nome
1	Michalowski, MJ;	2	Castro Ceron, JMC;	3	Wardlow, JL;
4	Karska, A;	5	Messias, H;	6	van der Werf, P;
7	Hunt, LK;	8	Baes, M;	9	Castro Tirado, AJ;
10	Gentile, G;	11	Hjorth, J;	12	Le Floc'h, E;
13	Perez Martinez, R;	14	Guelbenzu, AN;	15	Rasmussen, J;
16	Rizzo, JR;	17	Rossi, A;	18	Sanchez Portal, M;
19	Schady, P;	20	Sollerman, J;	21	Xu, D;

Grb 980425 Host: [C Ii], [O I], and Co Lines Reveal Recent Enhancement of Star Formation Due to Atomic Gas Inflow

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Grb 980425 Host: [C Ii], [O I], and Co Lines Reveal Recent Enhancement of Star Formation Due to Atomic Gas Inflow

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