Investigating the Source of Planck-Detected AME: High-Resolution Observations at 15 GHz
The Planck 28.5 GHz maps were searched for potential Anomalous Microwave Emission (AME) regions on the scale of ~3° or smaller, and several new regions of interest were selected. Ancillary data at both lower and higher frequencies were used to construct spectral energy distributions (SEDs), which se...
Saved in:
Main Authors: | , , , |
---|---|
Format: | Article |
Language: | English |
Published: |
Wiley
2013-01-01
|
Series: | Advances in Astronomy |
Online Access: | http://dx.doi.org/10.1155/2013/354259 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
_version_ | 1832552160839073792 |
---|---|
author | Yvette C. Perrott Anna M. M. Scaife Natasha Hurley-Walker Keith J. B. Grainge |
author_facet | Yvette C. Perrott Anna M. M. Scaife Natasha Hurley-Walker Keith J. B. Grainge |
author_sort | Yvette C. Perrott |
collection | DOAJ |
description | The Planck 28.5 GHz maps were searched for potential Anomalous Microwave Emission (AME) regions on the scale of ~3° or smaller, and several new regions of interest were selected. Ancillary data at both lower and higher frequencies were used to construct spectral energy distributions (SEDs), which seem to confirm an excess consistent with spinning dust models. Here we present higher resolution observations of two of these new regions with the Arcminute Microkelvin Imager Small Array (AMI SA) between 14 and 18 GHz to test for the presence of a compact (~10 arcmin or smaller) component. For AME-G107.1+5.2, dominated by the Hii region S140, we find evidence for the characteristic rising spectrum associated with either the spinning dust mechanism for AME or an ultra- /hypercompact Hii region across the AMI frequency band; however, for AME-G173.6+208 we find no evidence for AME on scales of ~2–10 arcmin. |
format | Article |
id | doaj-art-618fc512f83141758e84fee9d4f4a825 |
institution | Kabale University |
issn | 1687-7969 1687-7977 |
language | English |
publishDate | 2013-01-01 |
publisher | Wiley |
record_format | Article |
series | Advances in Astronomy |
spelling | doaj-art-618fc512f83141758e84fee9d4f4a8252025-02-03T05:59:27ZengWileyAdvances in Astronomy1687-79691687-79772013-01-01201310.1155/2013/354259354259Investigating the Source of Planck-Detected AME: High-Resolution Observations at 15 GHzYvette C. Perrott0Anna M. M. Scaife1Natasha Hurley-Walker2Keith J. B. Grainge3Astrophysics Group, Cavendish Laboratory, 19 J. J. Thomson Avenue, Cambridge CB3 0HE, UKSchool of Physics & Astronomy, University of Southampton, Highfield, Southampton SO17 1BJ, UKInternational Centre for Radio Astronomy Research, Curtin Institute of Radio Astronomy, 1 Turner Avenue, Technology Park, Bentley, Perth, WA 6845, AustraliaAstrophysics Group, Cavendish Laboratory, 19 J. J. Thomson Avenue, Cambridge CB3 0HE, UKThe Planck 28.5 GHz maps were searched for potential Anomalous Microwave Emission (AME) regions on the scale of ~3° or smaller, and several new regions of interest were selected. Ancillary data at both lower and higher frequencies were used to construct spectral energy distributions (SEDs), which seem to confirm an excess consistent with spinning dust models. Here we present higher resolution observations of two of these new regions with the Arcminute Microkelvin Imager Small Array (AMI SA) between 14 and 18 GHz to test for the presence of a compact (~10 arcmin or smaller) component. For AME-G107.1+5.2, dominated by the Hii region S140, we find evidence for the characteristic rising spectrum associated with either the spinning dust mechanism for AME or an ultra- /hypercompact Hii region across the AMI frequency band; however, for AME-G173.6+208 we find no evidence for AME on scales of ~2–10 arcmin.http://dx.doi.org/10.1155/2013/354259 |
spellingShingle | Yvette C. Perrott Anna M. M. Scaife Natasha Hurley-Walker Keith J. B. Grainge Investigating the Source of Planck-Detected AME: High-Resolution Observations at 15 GHz Advances in Astronomy |
title | Investigating the Source of Planck-Detected AME: High-Resolution Observations at 15 GHz |
title_full | Investigating the Source of Planck-Detected AME: High-Resolution Observations at 15 GHz |
title_fullStr | Investigating the Source of Planck-Detected AME: High-Resolution Observations at 15 GHz |
title_full_unstemmed | Investigating the Source of Planck-Detected AME: High-Resolution Observations at 15 GHz |
title_short | Investigating the Source of Planck-Detected AME: High-Resolution Observations at 15 GHz |
title_sort | investigating the source of planck detected ame high resolution observations at 15 ghz |
url | http://dx.doi.org/10.1155/2013/354259 |
work_keys_str_mv | AT yvettecperrott investigatingthesourceofplanckdetectedamehighresolutionobservationsat15ghz AT annammscaife investigatingthesourceofplanckdetectedamehighresolutionobservationsat15ghz AT natashahurleywalker investigatingthesourceofplanckdetectedamehighresolutionobservationsat15ghz AT keithjbgrainge investigatingthesourceofplanckdetectedamehighresolutionobservationsat15ghz |