John Goodricke, Edward Pigott, and Their Study of Variable Stars
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Catalogue of the Earl Marshal's Papers at Arundel
CONTENTS CONTENTS v FOREWORD by Sir Anthony Wagner, K.C.V.O., Garter King of Arms vii PREFACE ix LIST OF REFERENCES xi NUMERICAL KEY xiii COURT OF CHIVALRY Dated Cases 1 Undated Cases 26 Extracts from, or copies of, records relating to the Court; miscellaneous records concerning the Court or its officers 40 EARL MARSHAL Office and Jurisdiction 41 Precedence 48 Deputies 50 Dispute between Thomas, 8th Duke of Norfolk and Henry, Earl of Berkshire, 1719-1725/6 52 Secretaries and Clerks 54 COLLEGE OF ARMS General Administration 55 Commissions, appointments, promotions, suspensions, and deaths of Officers of Arms; applications for appointments as Officers of Arms; lists of Officers; miscellanea relating to Officers of Arms 62 Office of Garter King of Arms 69 Officers of Arms Extraordinary 74 Behaviour of Officers of Arms 75 Insignia and dress 81 Fees 83 Irregularities contrary to the rules of honour and arms 88 ACCESSIONS AND CORONATIONS Coronation of King James II 90 Coronation of King George III 90 Coronation of King George IV 90 Coronation of Queen Victoria 90 Coronation of King Edward VII and Queen Alexandra 90 Accession and Coronation of King George V and Queen Mary 96 Royal Accession and Coronation Oaths 97 Court of Claims 99 FUNERALS General 102 King George II 102 Augusta, Dowager Princess of Wales 102 King George III 102 King William IV 102 William Ewart Gladstone 103 Queen Victoria 103 King Edward VII 104 CEREMONIAL Precedence 106 Court Ceremonial; regulations; appointments; foreign titles and decorations 107 Opening of Parliament -
The Denver Observer December 2017
The Denver DECEMBER 2017 OBSERVER Messier 76, the Little Dumbbell Nebula, one of the deep-sky objects featured in this month’s “Skies.” Image © Joe Gafford. DECEMBER SKIES by Zachary Singer The Solar System of view in your ’scope will include the Moon’s Sky Calendar 3 Full Moon December will be a decent month for eastern section and the star, with plenty of 10 Last-Quarter Moon planetary events; though some planets are room. 17 New Moon slipping from view, others will take their I recommend you observe early—it 26 First-Quarter Moon place. We also have an occultation of Alde- should be a beautiful view, with the star a baran; as seen from Denver, the Moon will bright spark near the Moon’s edge, and over pass in front of the star at approximately the following minutes (they’ll go fast, just like In the Observer 4:06 PM, on the 30th. At that point, with the recent solar eclipse did), you can see the Moon move in its orbit around us, using the sunset still more than half an hour away, the President’s Message . .2 star won’t be visible to the naked eye, but it star for a benchmark. (Before 4:00 PM, look Society Directory. 2 should be in a telescope if you know where for Aldebaran outside the square, but along to look: Imagine a square drawn just large the diagonal from the Moon’s center to that Schedule of Events . 2 enough to touch the edges of the Moon, and lower-left edge.) About Denver Astronomical Society . -
Binocular Universe: You're My Hero! December 2010
Binocular Universe: You're My Hero! December 2010 Phil Harrington on't you just love a happy ending? I know I do. Picture this. Princess Andromeda, a helpless damsel in distress, chained to a rock as a ferocious D sea monster loomed nearby. Just when all appeared lost, our hero -- Perseus! -- plunges out of the sky, kills the monster, and sweeps up our maiden in his arms. Together, they fly off into the sunset on his winged horse to live happily ever after. Such is the stuff of myths and legends. That story, the legend of Perseus and Andromeda, was recounted in last month's column when we visited some binocular targets within the constellation Cassiopeia. In mythology, Queen Cassiopeia was Andromeda's mother, and the cause for her peril in the first place. Left: Autumn star map from Star Watch by Phil Harrington Above: Finder chart for this month's Binocular Universe. Chart adapted from Touring the Universe through Binoculars Atlas (TUBA), www.philharrington.net/tuba.htm This month, we return to the scene of the rescue, to our hero, Perseus. He stands in our sky to the east of Cassiopeia and Andromeda, should the Queen's bragging get her daughter into hot water again. The constellation's brightest star, Mirfak (Alpha [α] Persei), lies about two-thirds of the way along a line that stretches from Pegasus to the bright star Capella in Auriga. Shining at magnitude +1.8, Mirfak is classified as a class F5 white supergiant. It radiates some 5,000 times the energy of our Sun and has a diameter 62 times larger. -
Wynyard Planetarium & Observatory a Autumn Observing Notes
Wynyard Planetarium & Observatory A Autumn Observing Notes Wynyard Planetarium & Observatory PUBLIC OBSERVING – Autumn Tour of the Sky with the Naked Eye CASSIOPEIA Look for the ‘W’ 4 shape 3 Polaris URSA MINOR Notice how the constellations swing around Polaris during the night Pherkad Kochab Is Kochab orange compared 2 to Polaris? Pointers Is Dubhe Dubhe yellowish compared to Merak? 1 Merak THE PLOUGH Figure 1: Sketch of the northern sky in autumn. © Rob Peeling, CaDAS, 2007 version 1.2 Wynyard Planetarium & Observatory PUBLIC OBSERVING – Autumn North 1. On leaving the planetarium, turn around and look northwards over the roof of the building. Close to the horizon is a group of stars like the outline of a saucepan with the handle stretching to your left. This is the Plough (also called the Big Dipper) and is part of the constellation Ursa Major, the Great Bear. The two right-hand stars are called the Pointers. Can you tell that the higher of the two, Dubhe is slightly yellowish compared to the lower, Merak? Check with binoculars. Not all stars are white. The colour shows that Dubhe is cooler than Merak in the same way that red-hot is cooler than white- hot. 2. Use the Pointers to guide you upwards to the next bright star. This is Polaris, the Pole (or North) Star. Note that it is not the brightest star in the sky, a common misconception. Below and to the left are two prominent but fainter stars. These are Kochab and Pherkad, the Guardians of the Pole. Look carefully and you will notice that Kochab is slightly orange when compared to Polaris. -
Interferometric Observations of the Hierarchical Triple System Algol
The Astrophysical Journal, 705:436–445, 2009 November 1 doi:10.1088/0004-637X/705/1/436 C 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A. INTERFEROMETRIC OBSERVATIONS OF THE HIERARCHICAL TRIPLE SYSTEM ALGOL Sz. Csizmadia1,2,9, T. Borkovits3, Zs. Paragi2,4,P.Abrah´ am´ 5, L. Szabados5, L. Mosoni6,9, L. Sturmann7, J. Sturmann7, C. Farrington7, H. A. McAlister7, T. A. ten Brummelaar7, N. H. Turner7, and P. Klagyivik8 1 Institute of Planetary Research, DLR Rutherfordstr. 2 D-12489 Berlin, Germany 2 MTA Research Group for Physical Geodesy and Geodynamics, H-1585 Budapest, P.O. Box 585, Hungary; [email protected] 3 Baja Astronomical Observatory, H-6500 Baja, Szegedi ut,´ Kt. 766, Hungary 4 Joint Institute for VLBI in Europe, Postbus 2, 7990 AA Dwingeloo, Netherlands 5 Konkoly Observatory, H-1525 Budapest, P.O. Box 67, Hungary 6 Max-Planck-Institut fur¨ Astronomy, Konigstuhl¨ 17, D-69117 Heidelberg, Germany 7 Center for High Angular Resolution Astronomy, Georgia State University, P.O. Box 3969, Atlanta, GA 30302, USA 8 Department of Astronomy, Roland Eotv¨ os¨ University, H-1517 Budapest, P.O. Box 32, Hungary Received 2009 March 16; accepted 2009 September 11; published 2009 October 12 ABSTRACT Algol is a triple stellar system consisting of a close semidetached binary orbited by a third object. Due to the disputed spatial orientation of the close pair, the third body perturbation of this pair is a subject of much research. In this study, we determine the spatial orientation of the close pair orbital plane using the CHARA Array, a six-element optical/IR interferometer located on Mount Wilson, and state-of-the-art e-EVN interferometric techniques. -
Welsh Acheivements Brochure
WELSH ACHIEVEMENTS [ IN SCIENCE, TECHNOLOGY AND ENGINEERING ] ‘Our vision in Wales is of a learning country, where highly- skilled and highly-qualified people are employed in high- technology, high added-value companies.’ Professor John Harries, first chief scientific adviser for Wales, speaking in 2011 at the Welsh universities collaboration, research knowledge and expertise programme – Welsh Crucible. This publication is also available electronically from business.wales.gov.uk/innovation To discuss your innovation needs please call Business Wales on 03000 6 03000 or visit business.wales.gov.uk. Print ISBN 978 1 4734 0171 6 Printed on recycled paper Digital ISBN 978 1 4734 0169 3 WG16613 / G/MH/4578 / 0813 © Crown copyright 2013 2 On a global scale Wales is a small, but smart country, in which every opportunity has been taken to optimise resources, designs and processes. Shaped by landscape and culture it made its mark on the world through the maximisation of the great natural mineral wealth found here. Wales continues to make its mark through in-depth scientific and technical understanding and commercial innovation. From the past to the present an impressive list of achievements, many of which are the first of their kind in the world, have given Wales a great momentum for the future. CONTENTS 02 Foreword 05 Bioscience and Health 13 The Built Environment 20 Telecommunications and ICT 26 Creative Industries 35 Energy 41 Engineering 45 Environmental Sciences 50 Materials 56 Transport 64 People 74 Milestones 86 Conclusion 1 The modern world is increasingly made up of the products of the application of science, technology and engineering. -
Marketing Fragment 6 X 10.5.T65
Cambridge University Press 978-0-521-84013-2 - The Cambridge Companion to Alexander Pope Edited by Pat Rogers Index More information INDEX Main references are in bold type. AP = Alexander Pope. Achilles, 65–7, 69, 70, 73, 74, 78, 214, 217 Bacon, Francis, first Baron Verulam Addison, Joseph (1672–1719), author, 3, 7, (1561–1626), author, 17, 20 28, 29–30, 89, 105, 135, 146, 158, 202 Bank of England, 176 Cato, 28, 29 Barber, John (1675–1741), printer, 194 Aeschylus (525–456 bc), Greek dramatist, 80 Bathurst, Allen, first Earl (1684–1775), Agamemnon, 65, 66, 69, 70, 78 friend of AP, 162, 168–71, 194, 214 Ajax, 65, 73, 74 Bentley, Richard (1662–1742), classical Akenside, Mark (1721–70), poet, 216 scholar, 5, 72–4, 202 Allen, Ralph (1693–1764), businessman and Berkshire, 9, 105, 106, 111, 113, 161, 210 philanthropist, 162 Betterton, Thomas (1635–1710), actor, 1, “Amica”, 199 188 Ancients and Moderns, 72, 74, 79 Bevis Mount, Hampshire, 162 Anglicanism, 10, 121, 122, 126, 127, 128, Binfield, Berkshire, 4, 25, 29, 106, 107, 113, 130 161, 198 animal spirits, 218 Bion, Greek poet, 108 Anne, Queen (1665–1714), 4, 31, 90, 111, Blackmore, Sir Richard (1654–1729), 112, 119, 135, 233 physician and poet, 38, 69, 207, 215, Arbuthnot, John (1667–1735), physician and 216, 218 writer, 27, 31, 33, 35, 93, 143, 155, Blackwell, Thomas (1701–57), classical 158–9, 212, 219 scholar, 81 Arcadia, 9, 108, 111, 112, 116 Blenheim Palace, Oxfordshire, 165, 171 Ariosto, Ludovico (1474–1533), Italian Blount, Martha (1690–1763), friend of poet, 93 AP, 16, 26, 27, 35, 112, 113, 128, 169, Aristotle (384–322 bc), Greek 177, 180, 199, 205, 206 philosopher, 64 Blount, Teresa (1688–1759), Arnold, Matthew (1828–88), author, 50 gentlewoman, 26, 112, 113, 200, 206 Atterbury, Francis (1662–1732), Blunt, Sir John (1677–1733), South Sea churchman, 5, 31, 123, 134, 136–7, projector, 156 140, 157, Boileau, Nicolas Despreaux´ (1636–1711), 199 French poet, 78 Atterbury plot (1722–23), 5, 10, 134, Bolingbroke, Henry St John, first Viscount 136–7, 141, 144, 147 (1678–1751), politician, 4, 10, 22, Augustus (C. -
A Basic Requirement for Studying the Heavens Is Determining Where In
Abasic requirement for studying the heavens is determining where in the sky things are. To specify sky positions, astronomers have developed several coordinate systems. Each uses a coordinate grid projected on to the celestial sphere, in analogy to the geographic coordinate system used on the surface of the Earth. The coordinate systems differ only in their choice of the fundamental plane, which divides the sky into two equal hemispheres along a great circle (the fundamental plane of the geographic system is the Earth's equator) . Each coordinate system is named for its choice of fundamental plane. The equatorial coordinate system is probably the most widely used celestial coordinate system. It is also the one most closely related to the geographic coordinate system, because they use the same fun damental plane and the same poles. The projection of the Earth's equator onto the celestial sphere is called the celestial equator. Similarly, projecting the geographic poles on to the celest ial sphere defines the north and south celestial poles. However, there is an important difference between the equatorial and geographic coordinate systems: the geographic system is fixed to the Earth; it rotates as the Earth does . The equatorial system is fixed to the stars, so it appears to rotate across the sky with the stars, but of course it's really the Earth rotating under the fixed sky. The latitudinal (latitude-like) angle of the equatorial system is called declination (Dec for short) . It measures the angle of an object above or below the celestial equator. The longitud inal angle is called the right ascension (RA for short). -
October, 2011
IN THIS ISSUE: OCTOBER 2011 Event Calendar, News Notes Minutes of the September Meeting MVAS Reminders: Party-on MVAS Activities: On The Road Again Observer’s Notes: Variable Heroines MVAS Homework: M-76, Little Dumbbell Homework Charts: Algol, asteroid (15) Eunomia Constellation of the Month: Perseus November 2011 Sky Almanac Gallery: Comet Quest, Summer Photos Meteorite Editor: Phil Plante 1982 Mathews Rd. #2 Youngstown OH 44514 OCTOBER 2011 NEWS NOTES Newsletter of the Mahoning Valley Astronomical Society, Inc. The Big Ear. Lofar (Low Frequency Array) is a new kind of radio telescope. It can see radio waves with low frequencies, similar to those that give us FM radio. Rather than collecting MVAS CALENDAR signals from individual radio sources, Lofar continuously monitors large swathes of sky. Lofar is more sensitive to the OCT 22 Business meeting at the MVCO 8:00 PM longest observable radio waves than any other telescope. It can OCT 29 Halloween Party at the MVCO 7:00 PM see many billions of light years out into space, back to the time before the first stars formed, a few hundred million years after NOV17/18 Leonid Meteor watch. On your own? Midnight… the Big Bang. On Monday, September 21, 2011, Sweden's Minister for Education and Research, Jan Bjorklund, opened the NOV 19 Business meeting at YSU. Show at 8:00 PM Onsala Space Observatory's newest telescope; to become part NOV 26 Star Party at the MVCO. 7:00 PM till…. of Lofar, which is the world's largest radio telescope. The 192 new radio antennas at Onsala's Lofar station will be linked together with 47 similar stations over the whole of NATIONAL & REGIONAL EVENTS Europe, and sent over the Internet to a central supercomputer in OCT 24 - 30 CSPG Fall Star Party, held in Chiefland, FL . -
The Planets for 1955 24 Eclipses, 1955 ------29 the Sky and Astronomical Phenomena Month by Month - - 30 Phenomena of Jupiter’S S a Te Llite S
THE OBSERVER’S HANDBOOK FOR 1955 PUBLISHED BY The Royal Astronomical Society of Canada C. A. C H A N T, E d ito r RUTH J. NORTHCOTT, A s s is t a n t E d ito r DAVID DUNLAP OBSERVATORY FORTY-SEVENTH YEAR OF PUBLICATION P r i c e 50 C e n t s TORONTO 13 Ross S t r e e t Printed for th e Society By the University of Toronto Press THE ROYAL ASTRONOMICAL SOCIETY OF CANADA The Society was incorporated in 1890 as The Astronomical and Physical Society of Toronto, assuming its present name in 1903. For many years the Toronto organization existed alone, but now the Society is national in extent, having active Centres in Montreal and Quebec, P.Q.; Ottawa, Toronto, Hamilton, London, and Windsor, Ontario; Winnipeg, Man.; Saskatoon, Sask.; Edmonton, Alta.; Vancouver and Victoria, B.C. As well as nearly 1000 members of these Canadian Centres, there are nearly 400 members not attached to any Centre, mostly resident in other nations, while some 200 additional institutions or persons are on the regular mailing list of our publications. The Society publishes a bi-monthly J o u r n a l and a yearly O b s e r v e r ’s H a n d b o o k . Single copies of the J o u r n a l are 50 cents, and of the H a n d b o o k , 50 cents. Membership is open to anyone interested in astronomy. Annual dues, $3.00; life membership, $40.00. -
Download This Article in PDF Format
A&A 587, A30 (2016) Astronomy DOI: 10.1051/0004-6361/201526623 & c ESO 2016 Astrophysics Search for systemic mass loss in Algols with bow shocks A. Mayer1, R. Deschamps2,3, and A. Jorissen2 1 University of Vienna, Department of Astrophysics, Sternwartestraße 77, 1180 Wien, Austria e-mail: [email protected] 2 Institut d’Astronomie et d’Astrophysique, Université Libre de Bruxelles, CP 226, Av. F. Roosevelt 50, 1050 Brussels, Belgium 3 European Southern Observatory, Alonso de Cordova 3107, 19001 Casilla, Santiago, Chile Received 28 May 2015 / Accepted 24 December 2015 ABSTRACT Aims. Various studies indicate that interacting binary stars of Algol type evolve non-conservatively. However, direct detections of systemic mass loss in Algols have been scarce so far. We study the systemic mass loss in Algols by looking for the presence of infrared excesses originating from the thermal emission of dust grains, which is linked to the presence of a stellar wind. Methods. In contrast to previous studies, we make use of the fact that stellar and interstellar material is piled up at the edge of the astrosphere where the stellar wind interacts with the interstellar medium. We analyse WISE W3 12 μm and WISE W4 22 μmdataof Algol-type binary Be and B[e] stars and the properties of their bow shocks. From the stand-off distance of the bow shock we are able to determine the mass-loss rate of the binary system. Results. Although the velocities of the stars with respect to the interstellar medium are quite low, we find bow shocks present in two systems, namely π Aqr, and ϕ Per; a third system, CX Dra, shows a more irregular circumstellar environment morphology which might somehow be related to systemic mass loss. -
December 2019 BRAS Newsletter
A Monthly Meeting December 11th at 7PM at HRPO (Monthly meetings are on 2nd Mondays, Highland Road Park Observatory). Annual Christmas Potluck, and election of officers. What's In This Issue? President’s Message Secretary's Summary Outreach Report Asteroid and Comet News Light Pollution Committee Report Globe at Night Member’s Corner – The Green Odyssey Messages from the HRPO Friday Night Lecture Series Science Academy Solar Viewing Stem Expansion Transit of Murcury Edge of Night Natural Sky Conference Observing Notes: Perseus – Rescuer Of Andromeda, or the Hero & Mythology Like this newsletter? See PAST ISSUES online back to 2009 Visit us on Facebook – Baton Rouge Astronomical Society Baton Rouge Astronomical Society Newsletter, Night Visions Page 2 of 25 December 2019 President’s Message I would like to thank everyone for having me as your president for the last two years . I hope you have enjoyed the past two year as much as I did. We had our first Members Only Observing Night (MOON) at HRPO on Sunday, 29 November,. New officers nominated for next year: Scott Cadwallader for President, Coy Wagoner for Vice- President, Thomas Halligan for Secretary, and Trey Anding for Treasurer. Of course, the nominations are still open. If you wish to be an officer or know of a fellow member who would make a good officer contact John Nagle, Merrill Hess, or Craig Brenden. We will hold our annual Baton Rouge “Gastronomical” Society Christmas holiday feast potluck and officer elections on Monday, December 9th at 7PM at HRPO. I look forward to seeing you all there. ALCon 2022 Bid Preparation and Planning Committee: We’ll meet again on December 14 at 3:00.pm at Coffee Call, 3132 College Dr F, Baton Rouge, LA 70808, UPCOMING BRAS MEETINGS: Light Pollution Committee - HRPO, Wednesday December 4th, 6:15 P.M.