Visual Orbits of Spectroscopic Binaries with the CHARA Array
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Ioptron CEM40 Center-Balanced Equatorial Mount
iOptron®CEM40 Center-Balanced Equatorial Mount Instruction Manual Product CEM40 (#7400A series) and CEM40EC (#7400ECA series, as shown) Please read the included CEM40 Quick Setup Guide (QSG) BEFORE taking the mount out of the case! This product is a precision instrument. Please read the included QSG before assembling the mount. Please read the entire Instruction Manual before operating the mount. You must hold the mount firmly when disengaging the gear switches. Otherwise personal injury and/or equipment damage may occur. Any worm system damage due to improper operation will not be covered by iOptron’s limited warranty. If you have any questions please contact us at [email protected] WARNING! NEVER USE A TELESCOPE TO LOOK AT THE SUN WITHOUT A PROPER FILTER! Looking at or near the Sun will cause instant and irreversible damage to your eye. Children should always have adult supervision while using a telescope. 2 Table of Contents Table of Contents ........................................................................................................................................ 3 1. CEM40 Introduction ............................................................................................................................... 5 2. CEM40 Overview ................................................................................................................................... 6 2.1. Parts List ......................................................................................................................................... -
Proper Motion Analysis of the Jet of R Aquarii
A&A 424, 157–164 (2004) Astronomy DOI: 10.1051/0004-6361:20035866 & c ESO 2004 Astrophysics Proper motion analysis of the jet of R Aquarii K. Mäkinen1,H.J.Lehto1,2,R.Vainio3, and D. R. H. Johnson4 1 Tuorla Observatory, Väisäläntie 20, 21500 Piikkiö, Finland e-mail: [email protected] 2 Department of Physics, 20014 Turku University, Finland 3 Department of Physical Sciences, PO Box 64, 00014 University of Helsinki, Finland 4 Charterhouse, Godalming, Surrey, GU7 2DX, UK Received 15 December 2003 / Accepted 18 May 2004 Abstract. We have observed the jet of R Aquarii at high resolution with the VLA in 1992.83 and in 1999.78. Observations in the first epoch have resolved the base of the jet which shows a helical structure. We cannot detect the expected new jet component at either epoch. This does not disprove the idea of periodic ejection. Either the timing inferred from the acceleration models, or the assumed periastron passage is incorrect. Alternatively, a single new component cannot be resolved due to the dense core. Proper motion analysis of the jet components shows that previously derived acceleration models do not fit our new data. Indeed, the first ∼1 of the jet, both to north-east and south-west, appears fixed and has slowly moving shocks at the termination points, whereas the positions of the outer components fit best a ballistic orbit. We propose that the components are formed due to enhanced matter flow at periastron, accelerated during the first 1 and then ejected as bullets. Component A at a distance of ∼4 from the core has broken into two parts, similar to what was previously assumed to have happened to the outermost components B and D. -
August 2017 BRAS Newsletter
August 2017 Issue Next Meeting: Monday, August 14th at 7PM at HRPO nd (2 Mondays, Highland Road Park Observatory) Presenters: Chris Desselles, Merrill Hess, and Ben Toman will share tips, tricks and insights regarding the upcoming Solar Eclipse. What's In This Issue? President’s Message Secretary's Summary Outreach Report - FAE Light Pollution Committee Report Recent Forum Entries 20/20 Vision Campaign Messages from the HRPO Perseid Meteor Shower Partial Solar Eclipse Observing Notes – Lyra, the Lyre & Mythology Like this newsletter? See past issues back to 2009 at http://brastro.org/newsletters.html Newsletter of the Baton Rouge Astronomical Society August 2017 President’s Message August, 21, 2017. Total eclipse of the Sun. What more can I say. If you have not made plans for a road trip, you can help out at HRPO. All who are going on a road trip be prepared to share pictures and experiences at the September meeting. BRAS has lost another member, Bart Bennett, who joined BRAS after Chris Desselles gave a talk on Astrophotography to the Cajun Clickers Computer Club (CCCC) in January of 2016, Bart became the President of CCCC at the same time I became president of BRAS. The Clickers are shocked at his sudden death via heart attack. Both organizations will miss Bart. His obituary is posted online here: http://www.rabenhorst.com/obituary/sidney-barton-bart-bennett/ Last month’s meeting, at LIGO, was a success, even though there was not much solar viewing for the public due to clouds and rain for most of the afternoon. BRAS had a table inside the museum building, where Ben and Craig used material from the Night Sky Network for the public outreach. -
GEORGE HERBIG and Early Stellar Evolution
GEORGE HERBIG and Early Stellar Evolution Bo Reipurth Institute for Astronomy Special Publications No. 1 George Herbig in 1960 —————————————————————– GEORGE HERBIG and Early Stellar Evolution —————————————————————– Bo Reipurth Institute for Astronomy University of Hawaii at Manoa 640 North Aohoku Place Hilo, HI 96720 USA . Dedicated to Hannelore Herbig c 2016 by Bo Reipurth Version 1.0 – April 19, 2016 Cover Image: The HH 24 complex in the Lynds 1630 cloud in Orion was discov- ered by Herbig and Kuhi in 1963. This near-infrared HST image shows several collimated Herbig-Haro jets emanating from an embedded multiple system of T Tauri stars. Courtesy Space Telescope Science Institute. This book can be referenced as follows: Reipurth, B. 2016, http://ifa.hawaii.edu/SP1 i FOREWORD I first learned about George Herbig’s work when I was a teenager. I grew up in Denmark in the 1950s, a time when Europe was healing the wounds after the ravages of the Second World War. Already at the age of 7 I had fallen in love with astronomy, but information was very hard to come by in those days, so I scraped together what I could, mainly relying on the local library. At some point I was introduced to the magazine Sky and Telescope, and soon invested my pocket money in a subscription. Every month I would sit at our dining room table with a dictionary and work my way through the latest issue. In one issue I read about Herbig-Haro objects, and I was completely mesmerized that these objects could be signposts of the formation of stars, and I dreamt about some day being able to contribute to this field of study. -
Observing List
day month year Epoch 2000 local clock time: 4.00 Observing List for 24 7 2019 RA DEC alt az Constellation object mag A mag B Separation description hr min deg min 60 75 Andromeda Gamma Andromedae (*266) 2.3 5.5 9.8 yellow & blue green double star 2 3.9 42 19 73 111 Andromeda Pi Andromedae 4.4 8.6 35.9 bright white & faint blue 0 36.9 33 43 72 71 Andromeda STF 79 (Struve) 6 7 7.8 bluish pair 1 0.1 44 42 58 80 Andromeda 59 Andromedae 6.5 7 16.6 neat pair, both greenish blue 2 10.9 39 2 89 34 Andromeda NGC 7662 (The Blue Snowball) planetary nebula, fairly bright & slightly elongated 23 25.9 42 32.1 75 84 Andromeda M31 (Andromeda Galaxy) large sprial arm galaxy like the Milky Way 0 42.7 41 16 75 85 Andromeda M32 satellite galaxy of Andromeda Galaxy 0 42.7 40 52 75 82 Andromeda M110 (NGC205) satellite galaxy of Andromeda Galaxy 0 40.4 41 41 60 84 Andromeda NGC752 large open cluster of 60 stars 1 57.8 37 41 57 73 Andromeda NGC891 edge on galaxy, needle-like in appearance 2 22.6 42 21 89 173 Andromeda NGC7640 elongated galaxy with mottled halo 23 22.1 40 51 82 10 Andromeda NGC7686 open cluster of 20 stars 23 30.2 49 8 47 200 Aquarius 55 Aquarii, Zeta 4.3 4.5 2.1 close, elegant pair of yellow stars 22 28.8 0 -1 35 181 Aquarius 94 Aquarii 5.3 7.3 12.7 pale rose & emerald 23 19.1 -13 28 30 173 Aquarius 107 Aquarii 5.7 6.7 6.6 yellow-white & bluish-white 23 46 -18 41 26 221 Aquarius M72 globular cluster 20 53.5 -12 32 27 220 Aquarius M73 Y-shaped asterism of 4 stars 20 59 -12 38 40 181 Aquarius NGC7606 Galaxy 23 19.1 -8 29 28 219 Aquarius NGC7009 -
Ultraviolet Temporal Variability of the Peculiar Star R Aquarii S
Chapman University Chapman University Digital Commons Mathematics, Physics, and Computer Science Science and Technology Faculty Articles and Faculty Articles and Research Research 1995 Ultraviolet Temporal Variability of the Peculiar Star R Aquarii S. R. Meier USN, Research Laboratory Menas Kafatos Chapman University, [email protected] Follow this and additional works at: http://digitalcommons.chapman.edu/scs_articles Part of the Instrumentation Commons, and the Stars, Interstellar Medium and the Galaxy Commons Recommended Citation Meier, S.R., Kafatos, M. (1995) Ultraviolet Temporal Variability of the Peculiar Star R Aquarii, Astrophysical Journal, 451: 359-371. doi: 10.1086/176225 This Article is brought to you for free and open access by the Science and Technology Faculty Articles and Research at Chapman University Digital Commons. It has been accepted for inclusion in Mathematics, Physics, and Computer Science Faculty Articles and Research by an authorized administrator of Chapman University Digital Commons. For more information, please contact [email protected]. Ultraviolet Temporal Variability of the Peculiar Star R Aquarii Comments This article was originally published in Astrophysical Journal, volume 451, in 1995. DOI: 10.1086/176225 Copyright IOP Publishing This article is available at Chapman University Digital Commons: http://digitalcommons.chapman.edu/scs_articles/139 THE AsTROPHYSICAL JOURNAL, 451:359-371, 1995 September 20 © 1995. The American Astronomical Society. All rights reserved. Printed in U.S.A. 1995ApJ...451..359M -
Contents 2 Jan
By Martin Ratcliffe and Richard Talcott Sky Guide 2018 Mars shines brilliantly and looms large through telescopes this year as it puts on its finest show since 2003. NASA/JPL-CALTECH contents 2 Jan. 2018 Eclipse of the Blue Moon 3 Feb. 2018 Target galaxies these cool winter nights 4 March 2018 Catch Mercury at dusk 5 April 2018 The Lyre plays a sweet meteor song 6 May 2018 Jupiter rules spring nights 7 June 2018 Saturn’s rings on gorgeous display 8 July 2018 Red Planet renaissance 9 Aug. 2018 Prime time for the Perseids 10 Sept. 2018 Venus blazes in the evening twilight 11 Oct. 2018 An ice giant butts into the Ram Martin Ratcliffe provides professional 12 Nov. 2018 Juno at its best in 35 years planetarium development for Sky-Skan, Inc. Richard Talcott is a senior editor of Astronomy. 13 Dec. 2018 Making a swing past Earth 14 2019 Preview Looking ahead to next year ... A supplement to Astronomy magazine 618364 2018 Jan. S M T W T F S Eclipse of the 2 3 4 5 6 7 9 10 11 12 13 14 15 17 18 19 20 Blue Moon 21 22 23 25 26 27 28 29 30 anuary features two third of the country experience Full Moons, both of only the initial partial phases. which command our The Moon dips into Earth’s attention. The first dark umbral shadow at 1 Mercury is at great- comes New Year’s 6:48 a.m. EST (3:48 a.m. PST), est western elonga- night and arrives less than five but the Moon sets before total- tion (23°), 3 P.M. -
R Aquarii: Understanding the Mystery of Its Jets by Model Comparison Michelle Marie Risse Iowa State University
Iowa State University Capstones, Theses and Graduate Theses and Dissertations Dissertations 2009 R Aquarii: Understanding the mystery of its jets by model comparison Michelle Marie Risse Iowa State University Follow this and additional works at: https://lib.dr.iastate.edu/etd Part of the Physics Commons Recommended Citation Risse, Michelle Marie, "R Aquarii: Understanding the mystery of its jets by model comparison" (2009). Graduate Theses and Dissertations. 10565. https://lib.dr.iastate.edu/etd/10565 This Thesis is brought to you for free and open access by the Iowa State University Capstones, Theses and Dissertations at Iowa State University Digital Repository. It has been accepted for inclusion in Graduate Theses and Dissertations by an authorized administrator of Iowa State University Digital Repository. For more information, please contact [email protected]. R Aquarii: Understanding the mystery of its jets by model comparison by Michelle Marie Risse A thesis submitted to the graduate faculty in partial fulfillment of the requirements for the degree of MASTER OF SCIENCE Major: Astrophysics Program of Study Committee: Lee Anne Willson, Major Professor Steven D. Kawaler Craig A. Ogilvie David B. Wilson Iowa State University Ames, Iowa 2009 Copyright c Michelle Marie Risse, 2009. All rights reserved. ii TABLE OF CONTENTS LISTOFTABLES ................................... iv LISTOFFIGURES .................................. v CHAPTER1. Intent ................................. 1 CHAPTER2. Introduction ............................. 2 2.1 -
One of the Most Useful Accessories an Amateur Can Possess Is One of the Ubiquitous Optical Filters
One of the most useful accessories an amateur can possess is one of the ubiquitous optical filters. Having been accessible previously only to the professional astronomer, they came onto the marker relatively recently, and have made a very big impact. They are useful, but don't think they're the whole answer! They can be a mixed blessing. From reading some of the advertisements in astronomy magazines you would be correct in thinking that they will make hitherto faint and indistinct objects burst into vivid observ ability. They don't. What the manufacturers do not mention is that regardless of the filter used, you will still need dark and transparent skies for the use of the filter to be worthwhile. Don't make the mistake of thinking that using a filter from an urban location will always make objects become clearer. The first and most immediately apparent item on the downside is that in all cases the use of a filter reduces the amount oflight that reaches the eye, often quite sub stantially. The brightness of the field of view and the objects contained therein is reduced. However, what the filter does do is select specific wavelengths of light emitted by an object, which may be swamped by other wavelengths. It does this by suppressing the unwanted wavelengths. This is particularly effective in observing extended objects such as emission nebulae and planetary nebulae. In the former case, use a filter that transmits light around the wavelength of 653.2 nm, which is the spectral line of hydrogen alpha (Ha), and is the wavelength oflight respons ible for the spectacular red colour seen in photographs of emission nebulae. -
Instruction Manual
iOptron® GEM28 German Equatorial Mount Instruction Manual Product GEM28 and GEM28EC Read the included Quick Setup Guide (QSG) BEFORE taking the mount out of the case! This product is a precision instrument and uses a magnetic gear meshing mechanism. Please read the included QSG before assembling the mount. Please read the entire Instruction Manual before operating the mount. You must hold the mount firmly when disengaging or adjusting the gear switches. Otherwise personal injury and/or equipment damage may occur. Any worm system damage due to improper gear meshing/slippage will not be covered by iOptron’s limited warranty. If you have any questions please contact us at [email protected] WARNING! NEVER USE A TELESCOPE TO LOOK AT THE SUN WITHOUT A PROPER FILTER! Looking at or near the Sun will cause instant and irreversible damage to your eye. Children should always have adult supervision while observing. 2 Table of Content Table of Content ................................................................................................................................................. 3 1. GEM28 Overview .......................................................................................................................................... 5 2. GEM28 Terms ................................................................................................................................................ 6 2.1. Parts List ................................................................................................................................................. -
Double and Multiple Star Measurements at the Southern Sky with a 50Cm-Cassegrain and a Fast CCD Camera in 2008
Vol. 7 No. 2 April 1, 2011 Journal of Double Star Observations Page 64 Double and Multiple Star Measurements at the Southern Sky with a 50cm-Cassegrain and a Fast CCD Camera in 2008 Rainer Anton Altenholz/Kiel, Germany e-mail: rainer.anton”at”ki.comcity.de Abstract: Using a 50cm Cassegrain in Namibia, recordings of double and multiple stars were made with a fast CCD camera and a notebook computer. From superpositions of “lucky images”, measurements of 149 systems were obtained and compared with literature data. B/W and color images of some remarkable systems are also presented. 50 cm and focal ratio of f/9. It is located on a guest Introduction farm in Namibia and owned by the Internationale As has already been demonstrated in earlier pa- Amateur-Sternwarte (IAS) [1]. The setup for re- pers in this journal, the accuracy of double star cording was the same as I used earlier at home as measurements can be significantly improved by the well as at the southern sky [2-5]. In most recordings, technique of “lucky imaging”. Using short exposure I used a 2x Barlow lens (Televue) to extend the effec- times, only the best frames out of some thousands tive focal length to about 9 m (f/18). With my b/w- are registered and stacked. Thus, seeing effects are CCD camera (DMK21AF04, The Imaging Source) effectively reduced, and the resolution of a telescope with pixel size 5.6 µm square, this results in a reso- can be pushed to its limits, even under non-optimum lution of about 0.13 arcsec/pix. -
Star Dust Newsletter of National Capital Astronomers, Inc
Star Dust Newsletter of National Capital Astronomers, Inc. capitalastronomers.org May 2021 Volume 79, Issue 9 Celebrating 84 Years of Astronomy Radio Astronomy Observes Earth’s Ionosphere Next Meeting Dr. Joe Helmboldt When: Sat. May 8th, 2021 US Naval Research Laboratory (NRL) Time: 7:30 pm Where: Online (Zoom) Abstract: Ultraviolet photons from the Sun create a shroud of plasma See instructions for registering to participate in the meeting on Page 8. around the Earth within its upper atmosphere: the ionosphere. Any radio- frequency (RF) signal that passes through this region interacts with the Speaker: Joe Helmboldt free electrons there, delaying the signal. This is tantamount to a change Table of Contents in refractive index, so an RF-emitting object such as a satellite or a radio Preview of May 2021 Talk 1 galaxy will appear offset from its actual location on the sky. As the Recent Astronomy Highlights 2 electron density distribution evolves on a variety of time and length scales, this refractive effect also evolves, making it difficult to image Hubble 31st Birthday Image 2 astronomical radio sources. This is especially true at frequencies below Exploring the Sky 3 ~500 MHz, where this effect is the strongest. Sky Watchers 3 For several decades, this limited the size of interferometric imaging Stellar Mysteries 3 telescopes at these frequencies to <1 km. However, self-calibration NCA 2021-2022 Elections 4 methods developed in the 1980s and 1990s eliminated this barrier and Astronomical League 2021 allowed for the first sub-arcminute images below 100 MHz to be obtained Convention 4 in the early 2000s.