18 results with keyword: 'the stellar mass content of submillimeter selected galaxies'
The median of the stellar absolute H magnitude determined in this way for the z > 1.5 SMGs in our sample, including the upper limits for galaxies which had fewer than
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Unlike previous studies on leadership and development in Nigeria, which have observed that the system has been rendered unproductive by poor leadership, this article argues that
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GPM is a variation of Integrated Pest Management (IPM) with the goal to use fewer resources and chemicals using IPM practices. IPM focuses on pest prevention by eliminating
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Taking the dust emission as a proxy for dust-obscured star formation in our sources, our results imply that the SMG population at high redshift exhibits centrally concentrated
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We assume a burst timescale of 150 Myr, although note that this gives a conservative estimate since typical burst timescales of SMGs are estimated to be around 100 Myr (e.g., Simpson
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Castrol EDGE is Castrol’s premium, most advanced range of synthetic Engine Oils designed to meet the needs.. of newer, more technologically
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The search strategy and cost model enabled early selection o f promising alternatives thus enhancing optimiser efficiency and quality of QEPs produced. A number o
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interests in a closely held business) may be subject to "valuation discounts" for gift tax purposes, using less exemption than if the whole business was transferred at
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Typical H 2 SFEs compared with two optically selected samples: the local spiral galaxies of THINGS and COLD GASS galaxies of similar stellar mass. This comparison holds for
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Splitting the selected galaxies at different stellar mass thresholds, we measured the angular two-point correla- tion function and performed the halo modeling to link galaxies with
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6.1 Fits of Different Star Formation History Models to the SED of a Low- z SMG 153 6.2 Fits of Different Star Formation History Models to the SED of a High- z SMG 154 6.3
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This way, aqueous and ethanolic extracts from Campomanesia velutina leaves can act over crucial points of gout management: decrease uric acid serum lev- els by inhibiting
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Black hole mass versus host-galaxy total stellar mass for DES J0218 − 0430 in comparison to X-ray selected intermediate-redshift AGNs and local samples of AGNs and inactive
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The relation between stellar mass, Hubble type or stellar bar, and the H I content of galaxies as a function of look-back time can all be explored using both direct detections
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Furthermore, the underlying relationships between the stellar content of galaxies and their mass, ongoing star formation, internal structure, environment, and nuclear activity can
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Distributions of observable properties for the CGs identified in projection in the 2MASS XSC: number of members in the CG ( top-left panel ), percentage of members with
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Bottom: The stellar mass–magnitude relation for the same bands and redshifts. At fixed magnitude, the distribution of stellar mass is skewed towards low-mass galaxies, simply due to
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