OH in Messier 82

M K Argo; A Pedlar; T W B Muxlow; R J Beswick; S Aalto; K Wills; R S Booth; F Colomer; J-F Desmurs; P de Vicente; R Bachiller

OH in Messier 82

M K Argo, A Pedlar, T W B Muxlow, R J Beswick, S Aalto, K Wills, R S Booth, F Colomer, J-F Desmurs, P de Vicente, R Bachiller (Editor)

Research output: Chapter in Book/Conference proceeding › Conference contribution › peer-review

Abstract

Several new main line OH masers have been detected in the nearby starburst galaxy M82. Eight masers have been detected to 5σ, six of which are new detections. Observations covering both the 1665 and 1667 MHz lines with both the Very Large Array (VLA) and the Multi-Element Radio Linked Interferometer Network (MERLIN) have been used to accurately measure the positions and velocities of these features. Following analysis of the data, another six objects below 5σ, but with velocities consistent with the distribution inferred from the more certain detections, have been detected. These are classified as possible detections. (astro-ph/0412673)

Original language	English
Title of host publication	host publication
Editors	R Bachiller
Pages	151-152
Number of pages	2
Publication status	Published - 2004
Event	European VLBI Network on New Developments in VLBI Science and Technology - Duration: 1 Jan 1824 → … http://adsabs.harvard.edu/abs/2004evn..conf..151A

Conference

Conference	European VLBI Network on New Developments in VLBI Science and Technology
Period	1/01/24 → …
Internet address	http://adsabs.harvard.edu/abs/2004evn..conf..151A

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@inproceedings{d819911ab0824368a18eb25edb79afa3,

title = "OH in Messier 82",

abstract = "Several new main line OH masers have been detected in the nearby starburst galaxy M82. Eight masers have been detected to 5σ, six of which are new detections. Observations covering both the 1665 and 1667 MHz lines with both the Very Large Array (VLA) and the Multi-Element Radio Linked Interferometer Network (MERLIN) have been used to accurately measure the positions and velocities of these features. Following analysis of the data, another six objects below 5σ, but with velocities consistent with the distribution inferred from the more certain detections, have been detected. These are classified as possible detections. (astro-ph/0412673)",

author = "Argo, {M K} and A Pedlar and Muxlow, {T W B} and Beswick, {R J} and S Aalto and K Wills and Booth, {R S} and F Colomer and J-F Desmurs and {de Vicente}, P and R Bachiller",

year = "2004",

language = "English",

pages = "151--152",

editor = "R Bachiller",

booktitle = "host publication",

note = "European VLBI Network on New Developments in VLBI Science and Technology ; Conference date: 01-01-1824",

url = "http://adsabs.harvard.edu/abs/2004evn..conf..151A",

}

TY - GEN

T1 - OH in Messier 82

AU - Argo, M K

AU - Pedlar, A

AU - Muxlow, T W B

AU - Beswick, R J

AU - Aalto, S

AU - Wills, K

AU - Booth, R S

AU - Colomer, F

AU - Desmurs, J-F

AU - de Vicente, P

A2 - Bachiller, R

PY - 2004

Y1 - 2004

N2 - Several new main line OH masers have been detected in the nearby starburst galaxy M82. Eight masers have been detected to 5σ, six of which are new detections. Observations covering both the 1665 and 1667 MHz lines with both the Very Large Array (VLA) and the Multi-Element Radio Linked Interferometer Network (MERLIN) have been used to accurately measure the positions and velocities of these features. Following analysis of the data, another six objects below 5σ, but with velocities consistent with the distribution inferred from the more certain detections, have been detected. These are classified as possible detections. (astro-ph/0412673)

AB - Several new main line OH masers have been detected in the nearby starburst galaxy M82. Eight masers have been detected to 5σ, six of which are new detections. Observations covering both the 1665 and 1667 MHz lines with both the Very Large Array (VLA) and the Multi-Element Radio Linked Interferometer Network (MERLIN) have been used to accurately measure the positions and velocities of these features. Following analysis of the data, another six objects below 5σ, but with velocities consistent with the distribution inferred from the more certain detections, have been detected. These are classified as possible detections. (astro-ph/0412673)

M3 - Conference contribution

SP - 151

EP - 152

BT - host publication

T2 - European VLBI Network on New Developments in VLBI Science and Technology

Y2 - 1 January 1824

ER -

OH in Messier 82

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