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http://hdl.handle.net/2289/4452
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DC Field | Value | Language |
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dc.contributor.author | Bagla, Jasjeet S. | - |
dc.contributor.author | Nath, Biman B. | - |
dc.contributor.author | Padmanabhan, T. | - |
dc.date.accessioned | 2012-05-07T08:48:53Z | - |
dc.date.available | 2012-05-07T08:48:53Z | - |
dc.date.issued | 1997-08 | - |
dc.identifier.citation | Monthly Notices of the Royal Astronomical Society, 1997, Vol.289, p671 | en |
dc.identifier.issn | 0035-8711 | - |
dc.identifier.issn | 1365-2966 (Online) | - |
dc.identifier.uri | http://hdl.handle.net/2289/4452 | - |
dc.description | Restricted Access. An open-access version is available at arXiv.org (one of the alternative locations) | en |
dc.description.abstract | Large inhomogeneities in neutral hydrogen in the Universe can be detected at redshifts z<=10 using the redshifted 21-cm line emission. We use cosmological N-body simulations for dark matter and a simple model for baryonic collapse to estimate the signal expected from structures like protoclusters of galaxies at high redshifts. We study (i) the standard cold dark matter (CDM) model, (ii) a modified CDM model with less power at small scales, and (iii) a Lambda+CDM model in a universe with Omega_0+Omega_L=1. We show that it should be possible for the next generation of radio telescopes to detect such structures at a redshift of 3.34 with an integration of about 100 h. We also discuss possible schemes for enhancing signal-to-noise ratio to detect protocondensates at high redshifts. | en |
dc.language.iso | en | en |
dc.publisher | Royal Astronomical Society | en |
dc.relation.uri | http://adsabs.harvard.edu/abs/1997MNRAS.289..671B | en |
dc.relation.uri | http://arxiv.org/abs/astro-ph/9610267 | en |
dc.rights | 1997 Royal Astronomical Society | en |
dc.title | Neutral hydrogen at high redshifts as a probe of structure formation - III: Radio maps from N-body simulations | en |
dc.type | Article | en |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
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1997_MNRAS_V289_p671.pdf Restricted Access | Restricted Access | 1.16 MB | Adobe PDF | View/Open Request a copy |
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