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  • ASTROPHYSICS  (9)
  • feeding experiments  (4)
  • 2020-2022  (4)
  • 1980-1984  (9)
  • 1960-1964
  • 1950-1954
  • 1930-1934
  • 1
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    Zur Verwendung von Raps, Lupine und Ackerbohne im Forellenfutter (2021)
    In:  foe@vti.bund.de | http://aquaticcommons.org/id/eprint/6113 | 1240 | 2012-11-14 14:32:21 | 6113 | Bundesforschungsanstalt für Fischerei
    Details
    Publication Date: 2021-07-13
    Description: Johann Heinrich von Thunen-Institute, Federal Research Institute for Rural Areas, Forestry and Fisheries began publishing the Informationen aus der Fischereiforschung – Information on Fishery research in 2010
    Keywords: Aquaculture ; aquaculture ; substitute feed ; rapeseeds ; lupine ; field pea ; trout food ; feeding experiments ; growth
    Repository Name: AquaDocs
    Type: article , FALSE
    Format: application/pdf
    Format: application/pdf
    Format: 30-31
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  • 2
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    Krillmehl - ein geeigneter Fischmehlersatz im Forellenfutter (2021)
    In:  foe@vti.bund.de | http://aquaticcommons.org/id/eprint/6248 | 1240 | 2011-11-23 18:17:57 | 6248 | Bundesforschungsanstalt für Fischerei
    Details
    Publication Date: 2021-07-13
    Description: Johann Heinrich von Thunen-Institute, Federal Research Institute for Rural Areas, Forestry and Fisheries began publishing the Informationen aus der Fischereiforschung – Information on Fishery research in 2010
    Keywords: Aquaculture ; fish meal ; krill meal ; substitutes ; aquaculture ; Rainbow trout ; feeding experiments
    Repository Name: AquaDocs
    Type: article , FALSE
    Format: application/pdf
    Format: application/pdf
    Format: 97-98
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  • 3
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    Versuche zur Verwendung von Bakterienmehl im Forellenfutter (2021)
    In:  foe@vti.bund.de | http://aquaticcommons.org/id/eprint/6250 | 1240 | 2011-11-23 18:16:21 | 6250 | Bundesforschungsanstalt für Fischerei
    Details
    Publication Date: 2021-07-13
    Description: Johann Heinrich von Thunen-Institute, Federal Research Institute for Rural Areas, Forestry and Fisheries began publishing the Informationen aus der Fischereiforschung – Information on Fishery research in 2010
    Keywords: Aquaculture ; feeding experiments ; bacteria meal ; fish meal
    Repository Name: AquaDocs
    Type: article , FALSE
    Format: application/pdf
    Format: application/pdf
    Format: 98-99
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  • 4
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    Ersatz von Fischmehl durch Alkanhefe und Krillmehl im Forellenfutter (2021)
    In:  foe@vti.bund.de | http://aquaticcommons.org/id/eprint/6372 | 1240 | 2012-11-14 16:40:23 | 6372 | Bundesforschungsanstalt für Fischerei
    Details
    Publication Date: 2021-07-14
    Description: Johann Heinrich von Thunen-Institute, Federal Research Institute for Rural Areas, Forestry and Fisheries began publishing the Informationen aus der Fischereiforschung – Information on Fishery research in 2010
    Keywords: Aquaculture ; aquaculture ; feeding experiments ; nutritional properties ; food ; substitutes ; fishmeal ; trout feeding
    Repository Name: AquaDocs
    Type: article , FALSE
    Format: application/pdf
    Format: application/pdf
    Format: 21-22
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  • 5
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    Infrared emission line studies of the structure and excitation of H II regions (1982)
    In:  Other Sources
    Details
    Publication Date: 2011-08-18
    Description: Maps of five H II regions in one or more of the infrared fine-structure lines of Ne II (12.8 microns), Ar III (9.0 microns), and S IV (10.5 microns) have been obtained with angular resolutions ranging from 4 to 7 arcsec. The observations are used to discuss the morphology and excitation of these nebulae. Considerable diversity is found in the structures of the nebulae, probably resulting from differences in their ages and the circumstances of their formation. In all cases, more ionizing luminosity than would be provided by a single dominant ionizing star appears to be required, although uncertainties in the model nebulae make this conclusion uncertain.
    Keywords: ASTROPHYSICS
    Type: Astrophysical Journal; vol. 255
    Format: text
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  • 6
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    Infrared line and continuum views of G333.6-0.2 (1981)
    In:  Other Sources
    Details
    Publication Date: 2019-06-28
    Description: A 1-micron CCD picture and maps of the Ne II and Ar III fine-structure lines have been obtained in a region roughly one arcmin in size centered on the core of the compact H II region G333.6 - 0.2. The two emission-line maps show nearly identical intensity distributions, although much different fluxes. The maps are similar to the 1-micron picture smoothed to their angular resolutions. The infrared line of S IV also was detected and appears to have a spatial intensity distribution similar to that of the other fine-structure lines. The 1-micron picture reveals a small number of objects of nearly stellar appearance in the core, suggesting that G333.6 - 0.2 is powered by a compact cluster of sources. Stellar continuum radiation probably is responsible in part for the low equivalent width of the B-gamma line in the core.
    Keywords: ASTROPHYSICS
    Type: Astrophysical Journal; vol. 247
    Format: text
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  • 7
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    High spectral and spatial resolution observations of the 12.28 micron emission from H2 in the Orion Molecular Cloud (1982)
    In:  Other Sources
    Details
    Publication Date: 2019-06-28
    Description: The pure rotational S(2) line of H2 at 12.28 microns was sought in 44 positions in the Orion Molecular Cloud with 6-arcsec beams and 35 km/s spectral resolution; and it was detected in 27 positions. The lines are approximately symmetric and have full widths at half-maximum ranging from 100 km/s down to the resolution limit. The distribution of intensities and line shapes is largely consistent with that observed in the 2-micron hydrogen transitions; however, unexpectedly complex line profiles and point-to-point variations in line shapes appear, particularly in the region near IRc9.
    Keywords: ASTROPHYSICS
    Type: Astrophysical Journal; vol. 253
    Format: text
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  • 8
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    The abundances of neon, sulfur, and argon in planetary nebulae (1981)
    In:  Other Sources
    Details
    Publication Date: 2019-06-28
    Description: New infrared observations of Ne II, Ar III, and S IV are used in optical observations of other ionization states of the considered elements to evaluate the abundances of neon, argon, and sulfur in 18 planetary nebulae. Attention is also given to one or more of the infrared lines in 18 other nebulae. It is pointed out that S IV was detected in approximately 90% of the observed objects, while Ar III was found in about 80%, and Ne II in roughly one-third. It is noted that optical observations typically include only a limited region of the nebula, while the infrared measurements frequently involve integration over the entire nebular image.
    Keywords: ASTROPHYSICS
    Type: Astrophysical Journal; vol. 249
    Format: text
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  • 9
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    The structure of high-velocity gas in Orion and the possible role of IRc9 (1984)
    In:  Other Sources
    Details
    Publication Date: 2019-06-28
    Description: The spatial and velocity distribution of shocked gas in the Orion molecular cloud has been studied in detail through observations of near-infrared and middle-infrared H2 lines. It is argued that the observed structure requires either an asymmetric outflow or an inhomogeneous ambient molecular cloud, and that the second explanation appears the more likely. It is suggested that mild activity by IRc9, such as a T Tauri type wind or FU Orionis type flare, would be consistent with its apparent nature and could have caused the necessary density structure in the cloud.
    Keywords: ASTROPHYSICS
    Type: Astrophysical Journal, Part 1 (ISSN 0004-637X); 281; 205-208
    Format: text
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  • 10
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    The distribution of shocked gas in the bipolar nebulae CRL 2688 and CRL 618 (1984)
    In:  Other Sources
    Details
    Publication Date: 2019-06-28
    Description: Maps of the H2 emission from the bipolar nebulae CRL 2688 and CRL 618 are presented, along with a map of the 2.1-micron continuum emission from CRL 2688. The H2 emission is seen in the direction of the lobes of each nebula and not in between the lobes. From the distribution of the H2 and continuum emission, it is argued that the H2 is excited in shock waves produced in the lobes of the visible nebulae by fast winds from the central stars which overtake slower moving material lost in a slow wind during the red-giant phase of each object. These shocks may be similar to those seen in Herbig-Haro objects. The mass-loss rates for the fast winds in each object are estimated from the H2 data, and a brief discussion is given of the origin of these winds.
    Keywords: ASTROPHYSICS
    Type: Astrophysical Journal, Part 1 (ISSN 0004-637X); 280; 648-652
    Format: text
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