Journal article
Dust-correlated cm-wavelength continuum emission on translucent clouds ζ Oph and LDN 1780
- Abstract:
-
The diffuse cm-wave IR-correlated signal, the "anomalous" CMB foreground, is thought to arise in the dust in cirrus clouds. We present Cosmic Background Imager (CBI) cm-wave data of two translucent clouds, {\zeta} Oph and LDN 1780 with the aim of characterising the anomalous emission in the translucent cloud environment. In {\zeta} Oph, the measured brightness at 31 GHz is 2.4{\sigma} higher than an extrapolation from 5 GHz measurements assuming a free-free spectrum on 8 arcmin scales. The SE...
Expand abstract
- Publication status:
- Published
Actions
Access Document
- Publisher copy:
- 10.1111/j.1365-2966.2011.18562.x
Why is the content I wish to access not available via ORA?
Bibliographic data (the information relating to research outputs) and full-text items (e.g. articles, theses, reports, etc.) arrive in ORA from several different sources. Unfortunately we are not able to make available the full-text for every research output.
Please contact the ORA team (
) if you have queries regarding unavailable content OR if you are aware of a full-text copy we can make available.
) if you have queries regarding unavailable content OR if you are aware of a full-text copy we can make available.
Content may be unavailable for the following four reasons
-
Version unsuitable
-
We have not obtained a suitable full-text for a given research output. See this page for more information.
-
Recently completed
-
Sometimes content is held in ORA but is unavailable for a fixed period of time to comply with the policies and wishes of rights holders.
-
Permissions
-
All content made available in ORA should comply with relevant rights, such as copyright. See this page for more information.
-
Clearance
-
Some thesis volumes scanned as part of the digitisation scheme funded by Dr Leonard Polonsky are currently unavailable due to sensitive material or uncleared third-party copyright content. We are attempting to contact authors whose theses are affected.
Alternative access to the full-text
You may be able to access the full-text directly from the publisher's website using the 'Publisher Copy' link in the 'Links & Downloads' box from a research output's ORA record page. This method may require an institutional or individual subscription to the journal/resource.
Authors
Bibliographic Details
- Journal:
- Monthly Notices of the Royal Astronomical Society
- Volume:
- 414
- Issue:
- 3
- Pages:
- 2424-2435
- Publication date:
- 2011-02-21
- DOI:
- ISSN:
-
0035-8711
- Source identifiers:
-
161996
Item Description
- Keywords:
- Pubs id:
-
pubs:161996
- UUID:
-
uuid:0c0f5443-8315-46ac-bfa2-6a354765f843
- Local pid:
- pubs:161996
- Deposit date:
- 2012-12-19
Terms of use
- Copyright date:
- 2011
- Notes:
- 13 pages, 14 figures, 7 tables. Accepted for publication in MNRAS
If you are the owner of this record, you can report an update to it here: Report update to this record