Year 1904, I Am Unable to Give You Any Reliable Data.But I Hope the Aggregate Yield Will Equal That of Last Year
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Fishery Publications
124 COMMERCIAL FISHERIES REVIEW Vol. 26, o. RECENT FISHERY PUBLICATIONS SSR-Fish. No. 481 - Air and Water Temperatur e B a nd FISH AND WILDLIFE SERVICE Stream Flow Data, Convict Creek, Mono County Ca Iforma. 1950 to 1962. by Harry D. Kennedy, 50 pp., PUBLICATIONS Apnl 1964. Extent of Acid Mine Pollution in the United StateB Af THESE PROCESSED PUBLICATIONS ARE AVA I LABLE rREE r~ THE or. riCE or INrDRMATION, U. S. rlSH AND WILOLlrE SERVICE, WASHINGTON, fe1tmg1l='lsh and Wildlife , by-eowaz:a-r.Klnney,-cir· D. C. 20402. TYPES Of PUBLICATIONS ARE DESIGNATED AS rOLLDWS: cu ar ~:rpp.. 111us .. processed, June 1964. crs • CURRENT rlSHERY STATISTICS Of THE UNITEO STATES. THE rOLL 011 I NO MARIIET NEWS LEA rLETS ARE AVA I LABL£ ,~ THE rL • rlSHERY LEArLETS. rlSHERY MARKET NE\o'S""SEiiViCr;u.~u OF c.D>4HERCI A L FISHERIES ~NL • REPRINTS or RFPORTS ON fDREIGN fiSHERIES. RH. 510, 1815 N. FORT NYER OR., ARLINGTON, VA. 22209. SEP •• SE~RATES (REPRINTS) fRO~ CONNERCIAL fISHERIES.!!f.Yl.£!. SSR •• fiSH •• SPECIAL SCIENTifiC REPDRTS •• fISHERIES (LI~ITED DISTRIBUT ION). Number Title MNL-l1 - Fishing Industry 1I1Spaln, 1963 , 8 pp. Number Title MNL-26 - Taiwan Fisheries In 1963. 21 pp., CFS-3540 - Frozen Fishery Products, June 1964, 8 pp. MNL-40 - Moroccan Fishing Industry, 1962/63, 19 pp , CFS-3551 - Massachusetts Landings, January 1964.6 pp. CFS-3552 - Louisiana Landings, 1963 Annual Summary, THE FOLLOoII~ PUBLICATIONS ~E AVAILABLE Q!!U F~ THE m. 8 pp. CIFIC ~ HENTIONEO. CFS-3553 - Shrimp Landings, January 1964, 5 pp. CFS-3555 - Shrimp Landings, February 1964, 5 pp. -
Naming the Extrasolar Planets
Naming the extrasolar planets W. Lyra Max Planck Institute for Astronomy, K¨onigstuhl 17, 69177, Heidelberg, Germany [email protected] Abstract and OGLE-TR-182 b, which does not help educators convey the message that these planets are quite similar to Jupiter. Extrasolar planets are not named and are referred to only In stark contrast, the sentence“planet Apollo is a gas giant by their assigned scientific designation. The reason given like Jupiter” is heavily - yet invisibly - coated with Coper- by the IAU to not name the planets is that it is consid- nicanism. ered impractical as planets are expected to be common. I One reason given by the IAU for not considering naming advance some reasons as to why this logic is flawed, and sug- the extrasolar planets is that it is a task deemed impractical. gest names for the 403 extrasolar planet candidates known One source is quoted as having said “if planets are found to as of Oct 2009. The names follow a scheme of association occur very frequently in the Universe, a system of individual with the constellation that the host star pertains to, and names for planets might well rapidly be found equally im- therefore are mostly drawn from Roman-Greek mythology. practicable as it is for stars, as planet discoveries progress.” Other mythologies may also be used given that a suitable 1. This leads to a second argument. It is indeed impractical association is established. to name all stars. But some stars are named nonetheless. In fact, all other classes of astronomical bodies are named. -
Report of the Working Group on the Application of Genetics in Fisheries and Mariculture
,.· Mariculture Committee ICES CM 1996/F:2 ZJlo REPORT OF THE WORKING GROUP ON THE APPLICATION OF GENETICS IN FISHERIES AND MARICULTURE Faro, Portugal 19-23 February 1996 This report is not to be quoted without prior consuItation with the General Secretary. The document is areport of an expert group under the auspices ofthe International Council for the Exploration of the Sea and does not necessarily represent the views ofthe Council. International Council for the Exploration ofthe Sea Conseil International pour l'Exploration de la Mer Pala:gade 2-4 DK-1261 Copenhagen K Denmark • TABLE OF CONTENTS SECTION PAGE INTRODUCTION . 1.1 Attendance . 1.2 Working form .. 2 TERMS OF REFERENCE 1996 (C.Res.1995,2:28) 2 2.1a Selective fisheries 2 2.1 b Genetically modified organisms (GMO) 3 2.2 Management units / genetic resources 5 2.3a Genetic brood stock management 10 2.3b Good stocking practice 12 2.4 National activity reports and international cooperation 13 2.5 The 1997 ICESINASCO Symposium 13 3 WORKING GROUP BUSINESS 14 3.1 Comments on Working Group function 14 3.2 Comments on travel funds for WG members 14 3.3 Suggestions for WGAGFM Term of Reference and meetings in 1997 14 APPENDIX 1: National activity reports 16 APPENDIX 2: Terms ofReference 1996 (C.Res.1995, 2:28) 54 APPENDIX 3: Participants at the WGAGFM meeting in Faro 1996 55 APPENDIX 4: WGAGFM member list per April 1996 56 .. 1 INTRODUCTION Aeeordant with C.Res. 2:28 adopted at the 1995 Annual Scienee Conferenee in Aalborg, Denmark, the Working Group on the Applieation of Geneties in Fisheries and Marieulture (WGAGFM; Chairman J. -
Exoplanet.Eu Catalog Page 1 # Name Mass Star Name
exoplanet.eu_catalog # name mass star_name star_distance star_mass OGLE-2016-BLG-1469L b 13.6 OGLE-2016-BLG-1469L 4500.0 0.048 11 Com b 19.4 11 Com 110.6 2.7 11 Oph b 21 11 Oph 145.0 0.0162 11 UMi b 10.5 11 UMi 119.5 1.8 14 And b 5.33 14 And 76.4 2.2 14 Her b 4.64 14 Her 18.1 0.9 16 Cyg B b 1.68 16 Cyg B 21.4 1.01 18 Del b 10.3 18 Del 73.1 2.3 1RXS 1609 b 14 1RXS1609 145.0 0.73 1SWASP J1407 b 20 1SWASP J1407 133.0 0.9 24 Sex b 1.99 24 Sex 74.8 1.54 24 Sex c 0.86 24 Sex 74.8 1.54 2M 0103-55 (AB) b 13 2M 0103-55 (AB) 47.2 0.4 2M 0122-24 b 20 2M 0122-24 36.0 0.4 2M 0219-39 b 13.9 2M 0219-39 39.4 0.11 2M 0441+23 b 7.5 2M 0441+23 140.0 0.02 2M 0746+20 b 30 2M 0746+20 12.2 0.12 2M 1207-39 24 2M 1207-39 52.4 0.025 2M 1207-39 b 4 2M 1207-39 52.4 0.025 2M 1938+46 b 1.9 2M 1938+46 0.6 2M 2140+16 b 20 2M 2140+16 25.0 0.08 2M 2206-20 b 30 2M 2206-20 26.7 0.13 2M 2236+4751 b 12.5 2M 2236+4751 63.0 0.6 2M J2126-81 b 13.3 TYC 9486-927-1 24.8 0.4 2MASS J11193254 AB 3.7 2MASS J11193254 AB 2MASS J1450-7841 A 40 2MASS J1450-7841 A 75.0 0.04 2MASS J1450-7841 B 40 2MASS J1450-7841 B 75.0 0.04 2MASS J2250+2325 b 30 2MASS J2250+2325 41.5 30 Ari B b 9.88 30 Ari B 39.4 1.22 38 Vir b 4.51 38 Vir 1.18 4 Uma b 7.1 4 Uma 78.5 1.234 42 Dra b 3.88 42 Dra 97.3 0.98 47 Uma b 2.53 47 Uma 14.0 1.03 47 Uma c 0.54 47 Uma 14.0 1.03 47 Uma d 1.64 47 Uma 14.0 1.03 51 Eri b 9.1 51 Eri 29.4 1.75 51 Peg b 0.47 51 Peg 14.7 1.11 55 Cnc b 0.84 55 Cnc 12.3 0.905 55 Cnc c 0.1784 55 Cnc 12.3 0.905 55 Cnc d 3.86 55 Cnc 12.3 0.905 55 Cnc e 0.02547 55 Cnc 12.3 0.905 55 Cnc f 0.1479 55 -
Curt Teich Postcard Archives Towns and Cities
Curt Teich Postcard Archives Towns and Cities Alaska Aialik Bay Alaska Highway Alcan Highway Anchorage Arctic Auk Lake Cape Prince of Wales Castle Rock Chilkoot Pass Columbia Glacier Cook Inlet Copper River Cordova Curry Dawson Denali Denali National Park Eagle Fairbanks Five Finger Rapids Gastineau Channel Glacier Bay Glenn Highway Haines Harding Gateway Homer Hoonah Hurricane Gulch Inland Passage Inside Passage Isabel Pass Juneau Katmai National Monument Kenai Kenai Lake Kenai Peninsula Kenai River Kechikan Ketchikan Creek Kodiak Kodiak Island Kotzebue Lake Atlin Lake Bennett Latouche Lynn Canal Matanuska Valley McKinley Park Mendenhall Glacier Miles Canyon Montgomery Mount Blackburn Mount Dewey Mount McKinley Mount McKinley Park Mount O’Neal Mount Sanford Muir Glacier Nome North Slope Noyes Island Nushagak Opelika Palmer Petersburg Pribilof Island Resurrection Bay Richardson Highway Rocy Point St. Michael Sawtooth Mountain Sentinal Island Seward Sitka Sitka National Park Skagway Southeastern Alaska Stikine Rier Sulzer Summit Swift Current Taku Glacier Taku Inlet Taku Lodge Tanana Tanana River Tok Tunnel Mountain Valdez White Pass Whitehorse Wrangell Wrangell Narrow Yukon Yukon River General Views—no specific location Alabama Albany Albertville Alexander City Andalusia Anniston Ashford Athens Attalla Auburn Batesville Bessemer Birmingham Blue Lake Blue Springs Boaz Bobler’s Creek Boyles Brewton Bridgeport Camden Camp Hill Camp Rucker Carbon Hill Castleberry Centerville Centre Chapman Chattahoochee Valley Cheaha State Park Choctaw County -
A Market Analysis Towards the Further Development of Seaweed Aquaculture in Ireland
Part 1 A Market Analysis towards the Further Development of Seaweed Aquaculture in Ireland Principal authors Máirtín Walsh, BIM Lucy Watson, BIM Part 1 A Market Analysis towards the Further Development of Seaweed Aquaculture in Ireland. Principal authors Máirtín Walsh, BIM Lucy Watson, BIM Contributions from Geoff Robinson, BIM Christine Maggs, QUB Maeve Edwards, NUIG This document is an output of the project, PBA/SW/07/001(01), ‘Development and demonstration of viable hatchery and ongrowing methodologies for seaweed species with identified commercial potential’. This project is carried out under the Sea Change Strategy with the support of the Marine Institute and the Marine Research Sub-programme of the National Development Plan, 2007-2013. Table of Contents Page Executive Summary 3 1 Introduction 5 1.1 The Wild Resource 5 1.2 Project, PBA/SW/07/001(01) 5 1.3 Guiding Policy 6 1.4 The Opportunity 7 2 Industry Overview 9 3 Harvesting and Processing Seaweed to Market 12 3.1 Processing Palmaria palmata and Laminaria digitata 12 3.2 Adding Value through Processing 16 3.3 Milling / Grinding 18 3.4 Extraction 19 4 Markets 21 4.1 Food Products 21 4.2 Agricultural Products 21 4.3 Cosmetic Products 21 4.4 Pricing 22 5 Developing the Domestic Market for Seaweed Products 24 5.1 Increased Production Capacity 24 5.2 Improving Processing Capability 24 5.3 Supporting New Product Development 25 5.4 Provision of consumer information and in-store Promotional Material 25 5.5 Improving the Profile of Seaweed amongst Retailers 26 5.6 Expertise within the Seaweed -
Mètodes De Detecció I Anàlisi D'exoplanetes
MÈTODES DE DETECCIÓ I ANÀLISI D’EXOPLANETES Rubén Soussé Villa 2n de Batxillerat Tutora: Dolors Romero IES XXV Olimpíada 13/1/2011 Mètodes de detecció i anàlisi d’exoplanetes . Índex - Introducció ............................................................................................. 5 [ Marc Teòric ] 1. L’Univers ............................................................................................... 6 1.1 Les estrelles .................................................................................. 6 1.1.1 Vida de les estrelles .............................................................. 7 1.1.2 Classes espectrals .................................................................9 1.1.3 Magnitud ........................................................................... 9 1.2 Sistemes planetaris: El Sistema Solar .............................................. 10 1.2.1 Formació ......................................................................... 11 1.2.2 Planetes .......................................................................... 13 2. Planetes extrasolars ............................................................................ 19 2.1 Denominació .............................................................................. 19 2.2 Història dels exoplanetes .............................................................. 20 2.3 Mètodes per detectar-los i saber-ne les característiques ..................... 26 2.3.1 Oscil·lació Doppler ........................................................... 27 2.3.2 Trànsits -
Exoplanet.Eu Catalog Page 1 Star Distance Star Name Star Mass
exoplanet.eu_catalog star_distance star_name star_mass Planet name mass 1.3 Proxima Centauri 0.120 Proxima Cen b 0.004 1.3 alpha Cen B 0.934 alf Cen B b 0.004 2.3 WISE 0855-0714 WISE 0855-0714 6.000 2.6 Lalande 21185 0.460 Lalande 21185 b 0.012 3.2 eps Eridani 0.830 eps Eridani b 3.090 3.4 Ross 128 0.168 Ross 128 b 0.004 3.6 GJ 15 A 0.375 GJ 15 A b 0.017 3.6 YZ Cet 0.130 YZ Cet d 0.004 3.6 YZ Cet 0.130 YZ Cet c 0.003 3.6 YZ Cet 0.130 YZ Cet b 0.002 3.6 eps Ind A 0.762 eps Ind A b 2.710 3.7 tau Cet 0.783 tau Cet e 0.012 3.7 tau Cet 0.783 tau Cet f 0.012 3.7 tau Cet 0.783 tau Cet h 0.006 3.7 tau Cet 0.783 tau Cet g 0.006 3.8 GJ 273 0.290 GJ 273 b 0.009 3.8 GJ 273 0.290 GJ 273 c 0.004 3.9 Kapteyn's 0.281 Kapteyn's c 0.022 3.9 Kapteyn's 0.281 Kapteyn's b 0.015 4.3 Wolf 1061 0.250 Wolf 1061 d 0.024 4.3 Wolf 1061 0.250 Wolf 1061 c 0.011 4.3 Wolf 1061 0.250 Wolf 1061 b 0.006 4.5 GJ 687 0.413 GJ 687 b 0.058 4.5 GJ 674 0.350 GJ 674 b 0.040 4.7 GJ 876 0.334 GJ 876 b 1.938 4.7 GJ 876 0.334 GJ 876 c 0.856 4.7 GJ 876 0.334 GJ 876 e 0.045 4.7 GJ 876 0.334 GJ 876 d 0.022 4.9 GJ 832 0.450 GJ 832 b 0.689 4.9 GJ 832 0.450 GJ 832 c 0.016 5.9 GJ 570 ABC 0.802 GJ 570 D 42.500 6.0 SIMP0136+0933 SIMP0136+0933 12.700 6.1 HD 20794 0.813 HD 20794 e 0.015 6.1 HD 20794 0.813 HD 20794 d 0.011 6.1 HD 20794 0.813 HD 20794 b 0.009 6.2 GJ 581 0.310 GJ 581 b 0.050 6.2 GJ 581 0.310 GJ 581 c 0.017 6.2 GJ 581 0.310 GJ 581 e 0.006 6.5 GJ 625 0.300 GJ 625 b 0.010 6.6 HD 219134 HD 219134 h 0.280 6.6 HD 219134 HD 219134 e 0.200 6.6 HD 219134 HD 219134 d 0.067 6.6 HD 219134 HD -
The Role of Planet Accretion in Creating the Next Generation Of
Draft version November 2, 2018 A Preprint typeset using LTEX style emulateapj v. 08/22/09 THE ROLE OF PLANET ACCRETION IN CREATING THE NEXT GENERATION OF RED GIANT RAPID ROTATORS Joleen K. Carlberg1, Steven R. Majewski1, and Phil Arras1 Draft version November 2, 2018 ABSTRACT Rapid rotation in field red giant stars is a relatively rare but well-studied phenomenon; here we investigate the potential role of planet accretion in spinning up these stars. Using Zahn’s theory of tidal friction and stellar evolution models, we compute the decay of a planet’s orbit into its evolving host star and the resulting transfer of angular momentum into the stellar convective envelope. This experiment assesses the frequency of planet ingestion and rapid rotation on the red giant branch (RGB) for a sample of 99 known exoplanet host stars. We find that the known exoplanets are indeed capable of creating rapid rotators; however, the expected fraction due to planet ingestion is only 10% of the total seen in surveys of present-day red giants. Of the planets ingested, we find that those∼ with smaller initial semimajor axes are more likely to create rapid rotators because these planets are accreted when the stellar moment of inertia is smallest. We also find that many planets may be ingested prior to the RGB phase, contrary to the expectation that accretion would generally occur when the stellar radii expand significantly as giants. Finally, our models suggest that the rapid rotation signal from ingested planets is most likely to be seen on the lower RGB, which is also where alternative mechanisms for spin-up, e.g., angular momentum dredged up from the stellar core, do not operate. -
An Aquaculture Strategy for the Solway Prepared By
AN AQUACULTURE STRATEGY FOR THE SOLWAY PREPARED BY POSEIDON AQUATIC RESOURCE MANAGEMENT LTD and THE CENTRE FOR MARINE AND COASTAL STUDIES JUNE 2007 FUNDED AND COORDINATED BY 358-GBR An Aquaculture Strategy for the Solway Final Report TABLE OF CONTENTS Executive Summary 1 BACKGROUND.............................................................................................................1 1.1 INTRODUCTION ................................................................................................................................1 1.2 THE SOLWAY .....................................................................................................................................1 1.3 AQUACULTURE DEVELOPMENT IN THE UK AND SOLWAY ....................................................... 3 1.4 AIMS AND OBJECTIVES OF THE STRATEGY ...................................................................................5 1.5 SCOPE .................................................................................................................................................5 1.6 USE OF THE STRATEGY ....................................................................................................................6 1.7 METHODOLOGY ...............................................................................................................................7 2 THE EXISTING ENVIRONMENT ........................................................................... 8 2.1 POLICY AND REGULATORY FRAMEWORK ....................................................................................8 -
Extrasolar Planets and Brown Dwarfs Around A–F Type Stars
A&A 444, L21–L24 (2005) Astronomy DOI: 10.1051/0004-6361:200500176 & c ESO 2005 Astrophysics Extrasolar planets and brown dwarfs around A–F type stars II. A planet found with ELODIE around the F6V star HD 33564 F. Galland1,2, A.-M. Lagrange1,S.Udry2,A.Chelli1,F.Pepe2,J.-L.Beuzit1, and M. Mayor2 Letter to the Editor 1 Laboratoire d’Astrophysique de l’Observatoire de Grenoble, Université Joseph Fourier, BP 53, 38041 Grenoble, France e-mail: [email protected] 2 Observatoire de Genève, 51 Ch. des Maillettes, 1290 Sauverny, Switzerland Received 3 June 2005 / Accepted 3 September 2005 ABSTRACT We present here the detection of a planet orbiting around the F6V star HD 33564. The radial velocity measurements, obtained with the ELODIE echelle spectrograph at the Haute-Provence Observatory, show a variation with a period of 388 days. Assuming a primary mass of 1.25 M,the best Keplerian fit to the data leads to a minimum mass of 9.1 MJup for the companion. Key words. techniques: radial velocities – stars: binaries: spectroscopic – stars: early-type – stars: brown dwarfs – planetary systems 1. Introduction of a planet around one of the objects surveyed with ELODIE, HD 33564. Section 2 provides the stellar properties, the results Radial velocity surveys have lead to the detection of more of the radial velocity fit and related comments. In Sect. 3, we than 150 planets during the past decade1.Sofar,theyhave rule out other possible origins of the observed radial velocity been limited to solar and later-type stars (∼>F7), as it was variations. -
The Food Experience Castlemartyr Resort: the Bell Tower Restaurant
Free Ireland’s No1 Restaurant MEET THE LOAM GALWAY TEAM Food Tours ON IRELAND’S WILD ATLANTIC WAY Interview with Domini Kemp The Best ON BUILDING AN EMPIRE Recipes ON THE WILD ATLANTIC WAY TheGo WildThe Food Magazine,Food Food Summer 2019 ExperienceExperience THE HISTORY OF OYSTERS IN DONEGALPrefection Takes Time ysters were once a common food all along the European coastline, but overfishing in the 1800s resulted in them It Took us Obecoming a little known luxury. Despite this, Ireland is now one of the few 30 Years European countries where there are still wild, self-sustaining native oyster beds. About 100 years ago the first attempt was made to cultivate oysters in Ireland. It is only in the last 30 years that this has become successful. Two Since 1989 types of oyster are now cultivated in Ireland - the native European oyster oyster bank in the Lough…” These popular throughout the 1800s. Along or flat oyster (Ostrea edulis) and the oyster beds in Lough Foyle were with this rise in popularity the arrival of Irish rock oyster (Crassostrea gigas). referred to in 1846 and again in 1864, the railways allowed quick and efficient The Irish rock oyster was introduced to where forty or fifty boats were said transport to the main markets in Ireland in the late 1970s and is now the to have been engaged in the fishing Britain. Coupled with this, Irish oysters predominant oyster found in Ireland. compared to eight boats in 1836. were also being exploited for restocking The history of oyster-fishing in Ireland Locals could not avail of this food in the English and French fisheries is documented back to the 1500s, source during the famine period as resulting in significant impacts on though details of oyster fisheries in control of the fisheries was usually juvenile oysters.