VLA observations of 3 M33 supernova-remnants at 20 cm

WM Goss; F VIALLEFOND

doi:10.1007/BF02714994

VLA observations of 3 M33 supernova-remnants at 20 cm

WM Goss, F VIALLEFOND

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Three supernova remnants (SNR) have been mapped in the galaxy M33 with the Very Large Array* (VLA) at 20 cm. The angular resolution is ∼1.3 arcsec or ∼4 pc at a distance of 600 kpc and the rms noise is ∼0.04 mJy /beam. One of the radio sources shows evidence for a shell structure with a size of ∼15 pc, confirming the SNR nature of this source. The second object is extended and may well be a thick-shell SNR of size ∼12 pc. The third object is a small, presumably young SNR with a size of ∼4 pc.

Originele taal-2	English
Pagina's (van-tot)	145-151
Aantal pagina's	7
Tijdschrift	Journal of Astrophysics and Astronomy
Volume	6
Nummer van het tijdschrift	3
DOI's	https://doi.org/10.1007/BF02714994
Status	Published - sep-1985

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10.1007/BF02714994Licentie: Unspecified

VLA observations of three M 33 supernova remnants at 20 cmFinal publisher's version, 343 KBLicentie: Unspecified

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title = "VLA observations of 3 M33 supernova-remnants at 20 cm",

abstract = "Three supernova remnants (SNR) have been mapped in the galaxy M33 with the Very Large Array* (VLA) at 20 cm. The angular resolution is ∼1.3 arcsec or ∼4 pc at a distance of 600 kpc and the rms noise is ∼0.04 mJy /beam. One of the radio sources shows evidence for a shell structure with a size of ∼15 pc, confirming the SNR nature of this source. The second object is extended and may well be a thick-shell SNR of size ∼12 pc. The third object is a small, presumably young SNR with a size of ∼4 pc.",

author = "WM Goss and F VIALLEFOND",

year = "1985",

month = sep,

doi = "10.1007/BF02714994",

language = "English",

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pages = "145--151",

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TY - JOUR

T1 - VLA observations of 3 M33 supernova-remnants at 20 cm

AU - Goss, WM

AU - VIALLEFOND, F

PY - 1985/9

Y1 - 1985/9

N2 - Three supernova remnants (SNR) have been mapped in the galaxy M33 with the Very Large Array* (VLA) at 20 cm. The angular resolution is ∼1.3 arcsec or ∼4 pc at a distance of 600 kpc and the rms noise is ∼0.04 mJy /beam. One of the radio sources shows evidence for a shell structure with a size of ∼15 pc, confirming the SNR nature of this source. The second object is extended and may well be a thick-shell SNR of size ∼12 pc. The third object is a small, presumably young SNR with a size of ∼4 pc.

AB - Three supernova remnants (SNR) have been mapped in the galaxy M33 with the Very Large Array* (VLA) at 20 cm. The angular resolution is ∼1.3 arcsec or ∼4 pc at a distance of 600 kpc and the rms noise is ∼0.04 mJy /beam. One of the radio sources shows evidence for a shell structure with a size of ∼15 pc, confirming the SNR nature of this source. The second object is extended and may well be a thick-shell SNR of size ∼12 pc. The third object is a small, presumably young SNR with a size of ∼4 pc.

U2 - 10.1007/BF02714994

DO - 10.1007/BF02714994

M3 - Article

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SP - 145

EP - 151

JO - Journal of Astrophysics and Astronomy

JF - Journal of Astrophysics and Astronomy

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