Antropologiczne i socjologiczne spojrzenie na postać Ducha Parakleta w mowach pożegnalnych Jezusa (J 13-17)

Previous studies have suggested that salivary amylase and proline-rich protein are sorted differently when expressed in AtT-20 cells (Castle, A.M., L.E. Stahl, and J.D. Castle. 1992. J. Biol. Chem. 267:13093– 13100; Colomer, V., K. Lal, T.C. Hoops, and M.J. Rindler. 1994.EMBO (Eur. Mol. Biol. Organ.) J. 13:3711– 3719). We now show that both exocrine proteins behave similarly and enter the regulated secretory pathway as judged by immunolocalization and secretagogue- dependent stimulation of secretion. Analysis of stimulated secretion of newly synthesized proline-rich protein, amylase, and endogenous hormones indicates that the exogenous proteins enter the granule pool with about the same efficiency as the endogenous hormones. However, in contrast to the endogenous hormones, proline-rich protein and amylase are progressively removed from the granule pool during the process of granule maturation such that only small portions remain in mature granules where they colocalize with the stored hormones. The exogenous proteins that are not stored are recovered from the incubation medium and are presumed to have undergone constitutive-like secretion. These results point to a level of sorting for regulated secretion after entry of proteins into forming granules and indicate that retention is essential for efficient storage. Consequently, the critical role of putative sorting receptors for regulated secretion may be in retention rather than in granule entry.

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Longline Hook Selectivity for Branchiostegus japonicus (Houttuyn, 1782) and Dentex tumifrons (Temminck & Schlegel, 1843) in the East China Sea

Turkish Journal of Fisheries and Aquatic Sciences ◽

10.4194/1303-2712-v21_8_04 ◽

2021 ◽

Vol 21 (08) ◽

pp. 401-413

Author(s):

Guoqiang Xu ◽

Wenbin Zhu ◽

Yongdong Zhou ◽

Liuxiong Xu

Keyword(s):

East China Sea ◽

Reproductive Potential ◽

Mouth Opening ◽

Likelihood Method ◽

East China ◽

The East China Sea ◽

China Sea ◽

Total Length ◽

J 13 ◽

Branchiostegus Japonicus

Bottom longline fishing of red tilefish (Branchiostegus japonicus) is one of the most important commercial of fishing in the East China Sea. The present study aimed to investigate hook selectivity in B. japonicus and D. tumifrons, by means of experiments using three hook sizes (“J”: #15, #13 and #11) and was conducted in the East China Sea from June to August 2018. Altogether 602 B. japonicus fish and 858 D. tumifrons fish were caught. With respect to the size of the hook used, the total length-frequency varied significantly for both B. japonicus and D. tumifrons that were caught. The total length and four mouth parameters (upper and lower jaw length as well as height and width of mouth opening) of the two species showed a positive linear relationship. A logistic model created using the maximum likelihood method was used for elucidating hook selectivity; the best fit model with the minimum Akaike’s Information Criterion value was selected as the final model. The 50% selection lengths were 224.827 and 233.179 mm for B. japonicus; 201.461 and 202.603 mm for D. tumifrons using “J” #13 and “J” #11 hooks, respectively. To preserve the reproductive potential of younger fish in the stocks, the size of the “J” #13 hook was selected as the minimum hook size that should be used for the sustainable development of bottom longline fishing for B. japonicus and D. tumifrons.

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Data Qualification Report: Compostion of J-13 Well Water for Use on the Yucca Mountain Project

10.2172/895340 ◽

2000 ◽

Author(s):

T.L. Steinborn

Keyword(s):

Yucca Mountain ◽

Well Water ◽

J 13

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Corrosion Behavior of Carbon Steels Under Tuff Repository Environmental Conditions

MRS Proceedings ◽

10.1557/proc-44-287 ◽

1984 ◽

Vol 44 ◽

Author(s):

R. Daniel McCright ◽

H. Weiss

Keyword(s):

Stress Corrosion ◽

Carbon Steels ◽

Saturated Steam ◽

Nuclear Waste Repository ◽

Well Water ◽

General Corrosion ◽

Low Carbon ◽

Cast Irons ◽

J 13 ◽

Alloy Steels

AbstractCarbon steels may be used for borehole liners in a potential high-level nuclear waste repository in tuff in Nevada. Borehole liners are needed to facilitate emplacement of the waste packages and to facilitate retrieval of the packages, if required. Corrosion rates of low carbon structural steels AISI 1020 and ASTM A-36 were determined in J-13 well water and in saturated steam at 100°C. J-13 well water is representative of water which has percolated through the tuff horizon where the repository would be located. Tests were conducted in air-sparged J-13 water to attain stronger oxidizing conditions. A limited number of irradiation corrosion and stress corrosion tests were performed. Chromium-molybdenum alloy steels and cast irons were also tested. These materials showed lower general corrosion but were susceptible to stress corrosion cracking when welded.

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The molecular gas in Luminous Infrared Galaxies: a new emergent picture

Proceedings of the International Astronomical Union ◽

10.1017/s1743921313001117 ◽

2012 ◽

Vol 8 (S292) ◽

pp. 209-214

Author(s):

Padelis P. Papadopoulos ◽

Zhi-Yu Zhang ◽

Axel Weiss ◽

Paul van der Werf ◽

Kate Isaak ◽

...

Keyword(s):

Cosmic Ray ◽

Molecular Gas ◽

Infrared Galaxies ◽

Space Observatory ◽

Local Universe ◽

Star Forming ◽

Luminous Infrared Galaxies ◽

Physical Conditions ◽

J 13 ◽

Line Survey

AbstractResults from a large, multi-J CO, 13CO, and HCN line survey of Luminous Infrared Galaxies (LIRGs: LIR≥ 1010 L⊙) in the local Universe (z≤0.1), complemented by CO J=4–3 up to J=13–12 observations from the Herschel Space Observatory (HSO), paints a new picture for the average conditions of the molecular gas of the most luminous of these galaxies with turbulence and/or large cosmic ray (CR) energy densities UCR rather than far-UV/optical photons from star-forming sites as the dominant heating sources. Especially in ULIRGs (LIR>1012 L⊙) the Photon Dominated Regions (PDRs) can encompass at most a few % of their molecular gas mass while the large UCR∼ 103 UCR, Galaxy, and the strong turbulence in these merger/starbursts, can volumetrically heat much of their molecular gas to Tkin∼ (100-200) K, unhindered by the high dust extinctions. Moreover the strong supersonic turbulence in ULIRGs relocates much of their molecular gas at much higher average densities (≥104 cm−3) than in isolated spirals (∼ 102–103 cm−3). This renders low-J CO lines incapable of constraining the properties of the bulk of the molecular gas in ULIRGs, with substantial and systematic underestimates of its mass possible when only such lines are used. Finally a comparative study of multi-J HCN lines and CO SLEDs from J=1–0 up to J=13–12 of NGC 6240 and Arp 193 offers a clear example of two merger/starbursts whose similar low-J CO SLEDs, and LIR/LCO,1−0 and LHCN, 1−0/LCO,1-0 ratios (proxies of the so-called SF efficiency and dense gas mass fraction), yield no indications about their strongly diverging CO SLEDs beyond J=4–3, and ultimately the different physical conditions in their molecular ISM. The much larger sensitivity of ALMA and its excellent site in the Atacama desert now allows the observations necessary to assess the dominant energy sources of the molecular gas and its mass in LIRGs without depending on the low-J CO lines.

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Graphical Abstract: Chem. Eur. J. 13/2009

Chemistry - A European Journal ◽

10.1002/chem.200990039 ◽

2009 ◽

Vol 15 (13) ◽

pp. 3032-3039

Keyword(s):

J 13

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High-J CO Intensity Measurements for Galaxies Observed by the Herschel FTS

Proceedings of the International Astronomical Union ◽

10.1017/s1743921316007201 ◽

2015 ◽

Vol 11 (S315) ◽

pp. 26-29

Author(s):

Julia Kamenetzky ◽

Naseem Rangwala ◽

Jason Glenn ◽

Philip Maloney ◽

Alex Conley

Keyword(s):

Star Formation ◽

Galaxy Evolution ◽

Raw Material ◽

Molecular Gas ◽

Star Forming ◽

Star Forming Regions ◽

J 13 ◽

Systematic Effects ◽

Nearby Galaxies ◽

Co Emission

AbstractMolecular gas is the raw material for star formation and is commonly traced by the carbon monoxide (CO) molecule. The atmosphere blocks all but the lowest-J transitions of CO for observatories on the ground, but the launch of the Herschel Space Observatory revealed the CO emission of nearby galaxies from J = 4−3 to J = 13−12. Herschel showed that mid- and high-J CO lines in nearby galaxies are emitted from warm gas, accounting for approximately 10% of the molecular mass, but the majority of the CO luminosity. The energy budget of this warm, highly-excited gas is a significant window into the feedback interactions among molecular gas, star formation, and galaxy evolution. Likely, mechanical heating is required to explain the excitation. Such gas has also been observed in star forming regions within our galaxy.We have examined all ~300 spectra of galaxies from the Herschel Fourier Transform Spectrometer and measured line fluxes or upper limits for the CO J = 4−3 to J = 13−12, [CI], and [NII] 205 micron lines in ~200 galaxies, taking systematic effects of the FTS into account. We will present our line fitting method, illustrate trends available so far in this large sample, and preview the full 2-component radiative transfer likelihood modeling of the CO emission using an illustrative sample of 20 galaxies, including comparisons to well-resolved galactic regions. This work is a comprehensive study of mid- and high-J CO emission among a variety of galaxy types, and can be used as a resource for future (sub)millimeter studies of galaxies with ground-based instruments.

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