Mapping heavy elements in the supernova remnant G290.1-0.8

Murat HÜDAVERDİ

Makale detayları

Mapping heavy elements in the supernova remnant G290.1-0.8

Yazarlar:

Murat HÜDAVERDİ

Yayıncı:

TUBITAK

Ana Başlıklar:

Uygulamalı fizik

Dergi:

Turkish Journal of Physics 2018 Vol.42 Issue 4, pp.415-424

Belge Tipi:

Makale

Yayın Tarihi:

8/2018

Belge Dili:

İngilizce

Document ID (Org No.):

2000759239

Sıklık:

İki Aylık

eISSN:

1303-6122

pISSN:

1300-0101

Özet:

 


 
                         We present the imaging and spectroscopic study results of G290.1-0.8 Supernova Remnant (SNR) using the
Suzaku X-ray archival data. The SNR belongs to the mixed-morphology class with its centrally peaked asymmetric
X-ray core and distorted radio shell-like plasma. The X-ray spectra is well defined with isothermal plasma of kTe ∼ 0:5
keV. The radial profile shows enhanced elemental abundances. The EW maps reveal inhomogeneous asymmetric spatial
distribution of elemental abundances. The northeast of the SNR is bright in Ne, Mg, and Si. The EW maps are enhanced
in the direction of the X-ray elongation, suggesting that the distorted X-ray structure is dominated by a core-collapse
20∼25 M⊙ progenitor star ejecta.

                    

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Makale detayları

Mapping heavy elements in the supernova remnant G290.1-0.8

Yazarlar: Murat HÜDAVERDİ

Yayıncı: TUBITAK

Ana Başlıklar: Uygulamalı fizik

Dergi: Turkish Journal of Physics 2018 Vol.42 Issue 4, pp.415-424

Belge Tipi: Makale

Yayın Tarihi: 8/2018

Belge Dili: İngilizce

Document ID (Org No.): 2000759239

Sıklık: İki Aylık

eISSN: 1303-6122

pISSN: 1300-0101

Sayı

Yazarlar:

Murat HÜDAVERDİ

Yayıncı:

TUBITAK

Ana Başlıklar:

Uygulamalı fizik

Dergi:

Turkish Journal of Physics 2018 Vol.42 Issue 4, pp.415-424

Belge Tipi:

Makale

Yayın Tarihi:

8/2018

Belge Dili:

İngilizce

Document ID (Org No.):

2000759239

Sıklık:

İki Aylık

eISSN:

1303-6122

pISSN:

1300-0101