The Search For A Complex Molecule In A Selected Hot Core Region: A Rigorous Attempt To Confirm Trans-ethyl Methyl Ether Toward W51 E1/e2

Carroll, Brandon

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https://hdl.handle.net/2142/51159 Copy

Description

Title

The Search For A Complex Molecule In A Selected Hot Core Region: A Rigorous Attempt To Confirm Trans-ethyl Methyl Ether Toward W51 E1/e2

Author(s)

Carroll, Brandon

Contributor(s)

• Remijan, Anthony
• Blake, Geoffrey
• Ziurys, Lucy
• Apponi, Aldo J.
• McGuire, Brett A.

Issue Date

2014-06-18

Keyword(s)

Mini-symposium: Astronomical Molecular Spectroscopy in the Age of ALMA

Date of Ingest

• 2014-09-17T16:56:19Z
• 2015-04-14T18:42:18Z

Abstract

An extensive search has been conducted to confirm transitions of \textit{trans}-ethyl methyl ether (tEME), (C$_2$H$_5$OCH$_3$), toward the high mass star forming region W51 e1/e2 using the 12 m Telescope of the Arizona Radio Observatory (ARO) at 2 mm and 3 mm wavelengths. Typical peak to peak noise levels for the present observations of W51e1/e2 were between 10 mK to 30 mK, indicating an upper limit of the tEME column density of $\leq$ 1.5 $\times$ 10$^{15}$ cm$^{-2}$, this would make tEME at least a factor 2 times less abundant than dimethyl ether (CH$_3$OCH$_3$) toward W51 e1/e2. We have also performed an extensive search for this species toward the high mass star forming region Sgr B2(N-LMH) with the NRAO 100 m Green Bank Telescope (GBT). No transitions of tEME were detected and we were able to set an upper limit to the tEME column density of $\leq$ 4 $\times$ 10$^{14}$ cm$^{-2}$ toward Sgr B2(N-LMH). We will discuss these observations in the context of detecting large complex organic species toward star forming regions with next generation telescopes such as ALMA.

Publisher

International Symposium on Molecular Spectroscopy

Type of Resource

text

Genre of Resource

Conference Paper / Presentation

Language

English

Permalink

http://hdl.handle.net/2142/51159

DOI

https://doi.org/10.15278/isms.2014.WF09

Copyright and License Information

Copyright 2014 by the authors. Licensed under a Creative Commons Attribution 4.0 International License. http://creativecommons.org/licenses/by/4.0/

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