CONTENTS Volume 76 Nos 5 & 6 June 2017 in This Issue: NEWS
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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. -
Variable Star Section Circular
British Astronomical Association Variable Star Section Circular No 82, December 1994 CONTENTS A New Director 1 Credit for Observations 1 Submission of 1994 Observations 1 Chart Problems 1 Recent Novae Named 1 Z Ursae Minoris - A New R CrB Star? 2 The February 1995 Eclipse of 0¼ Geminorum 2 Computerisation News - Dave McAdam 3 'Stella Haitland, or Love and the Stars' - Philip Hurst 4 The 1994 Outburst of UZ Bootis - Gary Poyner 5 Observations of Betelgeuse by the SPA-VSS - Tony Markham 6 The AAVSO and the Contribution of Amateurs to VS Research Suspected Variables - Colin Henshaw 8 From the Literature 9 Eclipsing Binary Predictions 11 Summaries of IBVS's Nos 4040 to 4092 14 The BAA Instruments and Imaging Section Newsletter 16 Light-curves (TZ Per, R CrB, SV Sge, SU Tau, AC Her) - Dave McAdam 17 ISSN 0267-9272 Office: Burlington House, Piccadilly, London, W1V 9AG Section Officers Director Tristram Brelstaff, 3 Malvern Court, Addington Road, READING, Berks, RG1 5PL Tel: 0734-268981 Section Melvyn D Taylor, 17 Cross Lane, WAKEFIELD, Secretary West Yorks, WF2 8DA Tel: 0924-374651 Chart John Toone, Hillside View, 17 Ashdale Road, Cressage, Secretary SHREWSBURY, SY5 6DT Tel: 0952-510794 Computer Dave McAdam, 33 Wrekin View, Madeley, TELFORD, Secretary Shropshire, TF7 5HZ Tel: 0952-432048 E-mail: COMPUSERV 73671,3205 Nova/Supernova Guy M Hurst, 16 Westminster Close, Kempshott Rise, Secretary BASINGSTOKE, Hants, RG22 4PP Tel & Fax: 0256-471074 E-mail: [email protected] [email protected] Pro-Am Liaison Roger D Pickard, 28 Appletons, HADLOW, Kent TN11 0DT Committee Tel: 0732-850663 Secretary E-mail: [email protected] KENVAD::RDP Eclipsing Binary See Director Secretary Circulars Editor See Director Telephone Alert Numbers Nova and First phone Nova/Supernova Secretary. -
HET Publication Report HET Board Meeting 3/4 December 2020 Zoom Land
HET Publication Report HET Board Meeting 3/4 December 2020 Zoom Land 1 Executive Summary • There are now 420 peer-reviewed HET publications – Fifteen papers published in 2019 – As of 27 November, nineteen published papers in 2020 • HET papers have 29363 citations – Average of 70, median of 39 citations per paper – H-number of 90 – 81 papers have ≥ 100 citations; 175 have ≥ 50 cites • Wide angle surveys account for 26% of papers and 35% of citations. • Synoptic (e.g., planet searches) and Target of Opportunity (e.g., supernovae and γ-ray bursts) programs have produced 47% of the papers and 47% of the citations, respectively. • Listing of the HET papers (with ADS links) is given at http://personal.psu.edu/dps7/hetpapers.html 2 HET Program Classification Code TypeofProgram Examples 1 ToO Supernovae,Gamma-rayBursts 2 Synoptic Exoplanets,EclipsingBinaries 3 OneorTwoObjects HaloofNGC821 4 Narrow-angle HDF,VirgoCluster 5 Wide-angle BlazarSurvey 6 HETTechnical HETQueue 7 HETDEXTheory DarkEnergywithBAO 8 Other HETOptics Programs also broken down into “Dark Time”, “Light Time”, and “Other”. 3 Peer-reviewed Publications • There are now 420 journal papers that either use HET data or (nine cases) use the HET as the motivation for the paper (e.g., technical papers, theoretical studies). • Except for 2005, approximately 22 HET papers were published each year since 2002 through the shutdown. A record 44 papers were published in 2012. • In 2020 a total of fifteen HET papers appeared; nineteen have been published to date in 2020. • Each HET partner has published at least 14 papers using HET data. • Nineteen papers have been published from NOAO time. -
Winter Solstice 1988 No
Winter Solstice 1988 No. 61 ISSN 0715-4747 .. "'\,., ........ ~ UJ • oQ. en V) 01( U • • '" ;- r' j ,-: ~.: ':' : \ .:. ', ••' r:'l i. .', .• i .; l ;-i • C.A.S. Board of Directors President G. Michaud, U. de Montreal First Vice-President S. van den Bergh, D.A.O. Second Vice-President L. Higgs, D.R.A.O. Secretary C. Aikman, D.A.O. Treasurer J. Climenhaga, U. of Victoria Directors P. Martin, C.I.T.A. S. Pineault, U. Laval R. Roger, D.R.A.O. C.A.S. Committee Chairmen Awards P. Martin, C.I.T.A. Computing Facilities C. Pritchet, U. of Victoria Education R. Bochonko, U. of Manitoba Heritage P. Millman, H. I.A. Optical and Infrared Astronomy G. Harris, U. of Waterloo Radio Astronomy P. Dewdney, D.R.A.O. (acting) Small Grants C. Purton, D.R.A.O. Space Astronomy J. Hesser, D.A.O. Editor: Colin Scarfe Address: Department of Physics and Astronomy University of Victoria Victoria, B.C. V8W2Y2 Telephone: (604)721-7740 FAX: (604)721-7715 BITNET: SCARFE@UVPHYS Cassiopeia SECRETARY'S REPORT By now all members should have received their copies of the 1989 CASCA MEM· BERSHIP DIRECTORY. Please don't throw your old Direc tory away, as the CASCA Constitution is NOT reproduced in the new directory, as it was in the 1988 version. This is a good time then (although a better time would have been four weeks ago!) to let me know of any errors, alterations or omissions in the membership direc tory. One serious error No . 61 Winter Solstice 1988 that has already come to light is that electronic mail addresses on the CDNNET are listed in the directory as ending in the sub-domain .CA while in fact they should end in .CDN as given in last year's directory. -
Milestone Goto-Bino Series .Cdr
Kson MilestoneK Standard Alt/Az GOTO Mount INSTRUCTIONS CONTENT FOR KSON STANDARD ALT/AZ GOTO USER INTRODUCTION.................................................................................1 ACCESSORIES..................................................................................2 ASSEMBLY INSTRUCTIONS.............................................................3 FEATURES.........................................................................5 OPERATION MANUAL FOR SKYTOUCH CONTROLLER............... 6 KEY DESCRIPTION.................................................................................6 STATUS DESCRIPTION...........................................................................6 OPERATION PROCESS...........................................................................7 POWER ON......................................................................................7 WARNING........................................................................................7 ALIGNMENT STATUS........................................................................7 CHANGE THE DATE..................................................................7 CHANGE THE TIME...................................................................8 CHANGE THE SITE...................................................................8 ALIGNMENT.............................................................................9 NAVIGATION STATUS.....................................................................11 MENU STATUS................................................................................11 -
HET Publication Report HET Board Meeting 4/5 June 2020 Zoom Land
HET Publication Report HET Board Meeting 4/5 June 2020 Zoom Land 1 Executive Summary • There are now 410 peer-reviewed HET publications – Fifteen papers published in 2019 – As of 22 May, nine published papers in 2020 • HET papers have 28229 citations – Average of 69, median of 38 citations per paper – H-number of 90 – 76 papers have ≥ 100 citations; 170 have ≥ 50 cites • Wide angle surveys account for 27% of papers and 35% of citations. • Synoptic (e.g., planet searches) and Target of Opportunity (e.g., supernovae and γ-ray bursts) programs have produced 46% of the papers and 47% of the citations. • Listing of the HET papers (with ADS links) is given at http://personal.psu.edu/dps7/hetpapers.html 2 HET Program Classification Code TypeofProgram Examples 1 ToO Supernovae,Gamma-rayBursts 2 Synoptic Exoplanets,EclipsingBinaries 3 OneorTwoObjects HaloofNGC821 4 Narrow-angle HDF,VirgoCluster 5 Wide-angle BlazarSurvey 6 HETTechnical HETQueue 7 HETDEXTheory DarkEnergywithBAO 8 Other HETOptics Programs also broken down into “Dark Time”, “Light Time”, and “Other”. 3 Peer-reviewed Publications • There are now 410 journal papers that either use HET data or (nine cases) use the HET as the motivation for the paper (e.g., technical papers, theoretical studies). • Except for 2005, approximately 22 HET papers were published each year since 2002 through the shutdown. A record 44 papers were published in 2012. • In 2019 a total of fifteen HET papers appeared; nine have been published to date in 2019. • Each HET partner has published at least 14 papers using HET data. • Nineteen papers have been published from NOAO time. -
The COLOUR of CREATION Observing and Astrophotography Targets “At a Glance” Guide
The COLOUR of CREATION observing and astrophotography targets “at a glance” guide. (Naked eye, binoculars, small and “monster” scopes) Dear fellow amateur astronomer. Please note - this is a work in progress – compiled from several sources - and undoubtedly WILL contain inaccuracies. It would therefor be HIGHLY appreciated if readers would be so kind as to forward ANY corrections and/ or additions (as the document is still obviously incomplete) to: [email protected]. The document will be updated/ revised/ expanded* on a regular basis, replacing the existing document on the ASSA Pretoria website, as well as on the website: coloursofcreation.co.za . This is by no means intended to be a complete nor an exhaustive listing, but rather an “at a glance guide” (2nd column), that will hopefully assist in choosing or eliminating certain objects in a specific constellation for further research, to determine suitability for observation or astrophotography. There is NO copy right - download at will. Warm regards. JohanM. *Edition 1: June 2016 (“Pre-Karoo Star Party version”). “To me, one of the wonders and lures of astronomy is observing a galaxy… realizing you are detecting ancient photons, emitted by billions of stars, reduced to a magnitude below naked eye detection…lying at a distance beyond comprehension...” ASSA 100. (Auke Slotegraaf). Messier objects. Apparent size: degrees, arc minutes, arc seconds. Interesting info. AKA’s. Emphasis, correction. Coordinates, location. Stars, star groups, etc. Variable stars. Double stars. (Only a small number included. “Colourful Ds. descriptions” taken from the book by Sissy Haas). Carbon star. C Asterisma. (Including many “Streicher” objects, taken from Asterism. -
Globular Clusters, Though
Appendix: What You’re Looking At Early astronomers divided astronomical objects into three main types: planets, stars, and what were called mists or clouds; in Latin, nebulae. Stars had fixed positions relative to one another, but the planets moved about, and so the ancient Greeks called them wanderers, plan¯et¯es. The changing positions of the planets were hard to explain, and none of the Solar System models proposed bytheancientGreeksorRomansadequatelyexplainedthingssuchasretrograde motion. But even though they didn’t understand why the planets moved about, the Greeks and Romans both placed huge value on interpreting the movements of the planets. This is the art of astrology, a practice that has developed independently in many different cultures around the world. That stars were in some way similar to the Sun was something the ancient Greeks had guessed at, but it wasn’t until the nineteenth century and the invention of spec- troscopy that scientists could demonstrate that the light produced by the Sun was the similar to that produced by the stars. Over time different types of stars were identi- fied, and it soon became clear that the Sun was a relatively small and ordinary star by cosmic standards, even though it is vitally important to us. Nebulae posed particular problems for astronomers prior to the invention of the telescope. To the naked eye all nebulae look alike, nothing more than faint, misty patches of light. Only with the telescope was the diversity of nebulae revealed, but while they could be seen to be morphologically different, astronomers of the early modern era didn’t understand that a planetary nebula is a very different thing to something like the Great Nebula in Andromeda, what we’d today recognize as a galaxy. -
Fy05 Accomplishments and Fy06 Plans Helmut A. Abt
Appendix A NOAO SCIENTIFIC STAFF: FY05 ACCOMPLISHMENTS AND FY06 PLANS ¬New appointment in FY05 S Non-NSF (external) funding ±Term ended in FY05 HELMUT A. ABT, Emeritus Astronomer Research Interests Evolutionary stellar problems, stellar characteristics, publication studies FY05 Accomplishments Abt and C. Boonyarak (U. Thailand) studied rotation velocities of stars in binaries. It was known that those with periods shorter than several days all have synchronized rotational and orbital motions. They found that binaries with periods up to 500 days have reduced rotational velocities due to tidal interactions. Abt found that the eccentricities in binaries vary from zero in close binaries to an average of 0.5 in binaries with periods greater than 1000 days. In the initial formation of binaries, all eccentricities are equally probable. FY06 Plans Abt is trying to understand the hot inner disks that occur around, at any one time, one-quarter of the rapidly- rotating A dwarfs. These disks have no connection with the outer cool dust disks found around many stars like Vega and beta Pictoris. These disks come and go on time scales of decades. Such stars do not occur in the low-density Local Interstellar Bubble, so they are material accreted from the interstellar medium. Theoretical aspects of the physical processes is being done with M. Marlborough (U. Western Ontario). TAFT E. ARMANDROFF, Astronomer (Director, NOAO Gemini Science Center) Research Interests Stellar populations in the Galaxy and nearby galaxies; dwarf spheroidal galaxies; globular clusters FY05 Accomplishments Armandroff has been studying the dwarf spheroidal satellite galaxies of M31 in collaboration with Da Costa (RSAA/ANU), Pritzl (Macalester), and Jacoby (WIYN). -
Smithsonian Institution Fiscal Year ... Justification of Estimates Of
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321 the CELESCOPE CATALOG of ULTRAVIOLET OBSERVATIONS Robert J. Davis Smithsonian Astrophysical Observatory Cambridge, Massachus
321 THE CELESCOPE CATALOG OF ULTRAVIOLET OBSERVATIONS Robert J. Davis Smithsonian Astrophysical Observatory Cambridge, Massachusetts ABSTRACT The Smithsonian Astrophysical Observatory is using data obtained from approximately 7500 ultraviolet television pictures to compile The Celescope Catalog of Ultraviolet Observations described in this paper. This catalog lists the magnitude as observed in each of Celescope"s four ultraviolet color bands, the standard deviations of the observed ultraviolet mag- nitudes, positions, identifications, and ground-based magnitudes, colors, and spectral types for approxi- mately 5000 stars. A Preliminary Catalog of Celescope Ultraviolet Observations, containing data on about 500 stars, was distributed at the time this paper was presented. I. INTRODUCTION The Smithsonian Astrophysical Observatory operated an ultraviolet television photometer, called the Celescope exper- iment, in the second Orbiting Astronomical Observatory (OAO-2) of the National Aeronautics and Space Administration. During the 16 months that we operated Celescope (December 1968 through April 1970), we took 8784 television pictures, observ- ing about 1000 star fields once and about 700 more than once. We are now compiling the results from 7407 of these pictures into The Catalog of Celescope Ultraviolet Observations. Of the remaining 1377 pictures, 272 were not received, and 1105 were of quality too poor for processing. Included in this paper is a Preliminary Catalog of Cele- scope Ultraviolet Observations in the format in which we in- tend to publish the final catalog. We consider observational 322 SCIENTIFIC RESULTS OF OAO-2 material presented in this sample listing to be final. Since we are still reviewing the identifications and ground-based data, there may be a few changes in these quantities; however, the ultraviolet magnitudes will not change. -
EKCENTRIK Goto Mount最新版本091214
EklKipse Ekcentrik Mount INSTRUCTIONS CONTENT FOR EKCENTRIK USER INTRODUCTION.................................................................................1 ALL PARTS.........................................................................................2 ASSEMBLY INSTRUCTIONS.............................................................3 FEATURES.........................................................................5 OPERATION MANUAL FOR EKSTREAM KONTROLLER 30........... 6 KEY DESCRIPTION.................................................................................6 STATUS DESCRIPTION...........................................................................6 OPERATION PROCESS...........................................................................7 POWER ON......................................................................................7 WARNING........................................................................................7 ALIGNMENT STATUS........................................................................7 CHANGE THE DATE..................................................................7 CHANGE THE TIME...................................................................8 CHANGE THE SITE...................................................................8 ALIGNMENT.............................................................................9 NAVIGATION STATUS.....................................................................11 MENU STATUS................................................................................11