The Eastern Veil the Best of Monochrome
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Our Place in the Universe (239 Pages)
OUR PLACE IN THE uNIVERSE Norman k. Glendenning Lawrence Berkeley National Laboratiry World scientific Imperial College Press Published by Imperial College Press 57 Shelton Street Covent Garden London WC2H 9HE and World Scientific Publishing Co. Pte. Ltd. 5 Toh Tuck Link, Singapore 596224 USA office: 27 Warren Street, Suite 401-402, Hackensack, NJ 07601 UK office: 57 Shelton Street, Covent Garden, London WC2H 9HE Library of Congress Cataloging-in-Publication Data Glendenning, Norman K. Our place in the universe / Norman K. Glendenning. p. cm. Includes bibliographical references and index. ISBN-13 978-981-270-068-1 -- ISBN-10 981-270-068-4 ISBN-13 978-981-270-069-8 (pbk) -- ISBN-10 981-270-069-2 (pbk) 1. Cosmology. 2. Galaxies--Formation. 3. Galaxies--Evolution. 4. Astrophysics. 5. Solar system--Origin. I. Title. QB981 .G585 2007 523.1--dc22 British Library Cataloguing-in-Publication Data A catalogue record for this book is available from the British Library. Cover picture: The Horsehead is a reflection nebula; it is located in the much larger Orion Nebula, an immense molecular cloud of primordial hydrogen and helium, together dust cast off by the surfaces of stars. The clouds that form the Horsehead are illuminated from behind by a stellar nursery of young bright stars. Credit: Photo taken at Mauna Kea, Hawaii with the Canada-France-Hawaii Telescope. Copyright © 2007 by Imperial College Press and World Scientific Publishing Co. Pte. Ltd. All rights reserved. This book, or parts thereof, may not be reproduced in any form or by any means, electronic or mechanical, including photocopying, recording or any information storage and retrieval system now known or to be invented, without written permission from the Publisher. -
Polarimetric Properties of Blazars Caught by the WEBT
galaxies Review Polarimetric Properties of Blazars Caught by the WEBT Claudia M. Raiteri * and Massimo Villata INAF, Osservatorio Astrofisico di Torino, via Osservatorio 20, I-10025 Pino Torinese, Italy; [email protected] * Correspondence: [email protected] Abstract: Active galactic nuclei come in many varieties. A minority of them are radio-loud, and exhibit two opposite prominent plasma jets extending from the proximity of the supermassive black hole up to megaparsec distances. When one of the relativistic jets is oriented closely to the line of sight, its emission is Doppler beamed and these objects show extreme variability properties at all wavelengths. These are called “blazars”. The unpredictable blazar variability, occurring on a continuous range of time-scales, from minutes to years, is most effectively investigated in a multi-wavelength context. Ground-based and space observations together contribute to give us a comprehensive picture of the blazar emission properties from the radio to the g-ray band. Moreover, in recent years, a lot of effort has been devoted to the observation and analysis of the blazar polarimetric radio and optical behaviour, showing strong variability of both the polarisation degree and angle. The Whole Earth Blazar Telescope (WEBT) Collaboration, involving many tens of astronomers all around the globe, has been monitoring several blazars since 1997. The results of the corresponding data analysis have contributed to the understanding of the blazar phenomenon, particularly stressing the viability of a geometrical interpretation of the blazar variability. We review here the most significant polarimetric results achieved in the WEBT studies. Keywords: active galactic nuclei; blazars; jets; polarimetry Citation: Raiteri, C.M.; Villata, M. -
A Study of Ancient Khmer Ephemerides
A study of ancient Khmer ephemerides François Vernotte∗ and Satyanad Kichenassamy** November 5, 2018 Abstract – We study ancient Khmer ephemerides described in 1910 by the French engineer Faraut, in order to determine whether they rely on observations carried out in Cambodia. These ephemerides were found to be of Indian origin and have been adapted for another longitude, most likely in Burma. A method for estimating the date and place where the ephemerides were developed or adapted is described and applied. 1 Introduction Our colleague Prof. Olivier de Bernon, from the École Française d’Extrême Orient in Paris, pointed out to us the need to understand astronomical systems in Cambo- dia, as he surmised that astronomical and mathematical ideas from India may have developed there in unexpected ways.1 A proper discussion of this problem requires an interdisciplinary approach where history, philology and archeology must be sup- plemented, as we shall see, by an understanding of the evolution of Astronomy and Mathematics up to modern times. This line of thought meets other recent lines of research, on the conceptual evolution of Mathematics, and on the definition and measurement of time, the latter being the main motivation of Indian Astronomy. In 1910 [1], the French engineer Félix Gaspard Faraut (1846–1911) described with great care the method of computing ephemerides in Cambodia used by the horas, i.e., the Khmer astronomers/astrologers.2 The names for the astronomical luminaries as well as the astronomical quantities [1] clearly show the Indian origin ∗F. Vernotte is with UTINAM, Observatory THETA of Franche Comté-Bourgogne, University of Franche Comté/UBFC/CNRS, 41 bis avenue de l’observatoire - B.P. -
Navigating North America
deep-sky wonders by sue french Navigating North America the north america nebula is one of the most impres- NGC 6997 is the most obvious cluster within the confines sive nebulae glowing in our sky. This nebula’s remarkable of the North America Nebula. To me, it looks as though it’s resemblance to the North American continent makes it bet- been plunked down on the border between Ohio and West ter known by its common name — bestowed not by a resi- Virginia. Putting 4.8-magnitude 57 Cygni at the western dent of North America, but by German astrono- edge of a low-power eyepiece field should bring NGC 6997 Knowing mer Max Wolf. In 1890 Wolf became the first into view. My 4.1-inch scope at 17× displays a dusting of person to photograph the North America Nebula, very faint stars. At 47×, it’s a pretty cluster, rich in faint your and for many years this remained the only way to stars, spanning 10′. Through my 10-inch reflector, I count geography fully appreciate its distinctive shape. With today’s 40 stars, mostly of magnitude 11 and 12. Many are abundance of short-focal-length telescopes and arranged in two incomplete circles, one inside the other. puts you wide-field eyepieces, we can more readily enjoy Is NGC 6997 actually involved in the North America one step this large nebula visually. Nebula? It’s difficult to tell because the distances are poorly The North America Nebula, NGC 7000 or Cald- known. A journal article earlier this year puts NGC 6997 at ahead in well 20, is certainly easy to locate. -
BRAS Newsletter August 2013
www.brastro.org August 2013 Next meeting Aug 12th 7:00PM at the HRPO Dark Site Observing Dates: Primary on Aug. 3rd, Secondary on Aug. 10th Photo credit: Saturn taken on 20” OGS + Orion Starshoot - Ben Toman 1 What's in this issue: PRESIDENT'S MESSAGE....................................................................................................................3 NOTES FROM THE VICE PRESIDENT ............................................................................................4 MESSAGE FROM THE HRPO …....................................................................................................5 MONTHLY OBSERVING NOTES ....................................................................................................6 OUTREACH CHAIRPERSON’S NOTES .........................................................................................13 MEMBERSHIP APPLICATION .......................................................................................................14 2 PRESIDENT'S MESSAGE Hi Everyone, I hope you’ve been having a great Summer so far and had luck beating the heat as much as possible. The weather sure hasn’t been cooperative for observing, though! First I have a pretty cool announcement. Thanks to the efforts of club member Walt Cooney, there are 5 newly named asteroids in the sky. (53256) Sinitiere - Named for former BRAS Treasurer Bob Sinitiere (74439) Brenden - Named for founding member Craig Brenden (85878) Guzik - Named for LSU professor T. Greg Guzik (101722) Pursell - Named for founding member Wally Pursell -
Infrared Spectroscopy of Nearby Radio Active Elliptical Galaxies
The Astrophysical Journal Supplement Series, 203:14 (11pp), 2012 November doi:10.1088/0067-0049/203/1/14 C 2012. The American Astronomical Society. All rights reserved. Printed in the U.S.A. INFRARED SPECTROSCOPY OF NEARBY RADIO ACTIVE ELLIPTICAL GALAXIES Jeremy Mould1,2,9, Tristan Reynolds3, Tony Readhead4, David Floyd5, Buell Jannuzi6, Garret Cotter7, Laura Ferrarese8, Keith Matthews4, David Atlee6, and Michael Brown5 1 Centre for Astrophysics and Supercomputing Swinburne University, Hawthorn, Vic 3122, Australia; [email protected] 2 ARC Centre of Excellence for All-sky Astrophysics (CAASTRO) 3 School of Physics, University of Melbourne, Melbourne, Vic 3100, Australia 4 Palomar Observatory, California Institute of Technology 249-17, Pasadena, CA 91125 5 School of Physics, Monash University, Clayton, Vic 3800, Australia 6 Steward Observatory, University of Arizona (formerly at NOAO), Tucson, AZ 85719 7 Department of Physics, University of Oxford, Denys, Oxford, Keble Road, OX13RH, UK 8 Herzberg Institute of Astrophysics Herzberg, Saanich Road, Victoria V8X4M6, Canada Received 2012 June 6; accepted 2012 September 26; published 2012 November 1 ABSTRACT In preparation for a study of their circumnuclear gas we have surveyed 60% of a complete sample of elliptical galaxies within 75 Mpc that are radio sources. Some 20% of our nuclear spectra have infrared emission lines, mostly Paschen lines, Brackett γ , and [Fe ii]. We consider the influence of radio power and black hole mass in relation to the spectra. Access to the spectra is provided here as a community resource. Key words: galaxies: elliptical and lenticular, cD – galaxies: nuclei – infrared: general – radio continuum: galaxies ∼ 1. INTRODUCTION 30% of the most massive galaxies are radio continuum sources (e.g., Fabbiano et al. -
Discovery of a Pulsar Wind Nebula Candidate in the Cygnus Loop
Discovery of a Pulsar Wind Nebula Candidate in the Cygnus Loop 2 3 S Satoru Katsuda" Hiroshi Tsunemi , Koji Mori , Hiroyuki Uchida" Robert Petre , Shin'ya 1 Yamada , and Thru Tamagawa' ABSTRACT We report on a discovery of a diffuse nebula containing a pointlike source in the southern blowout region of the Cygnus Loop supernova remnant, based on Suzaku and XMM-Newton observations. The X-ray spectra from the nebula and the pointlike source are well represented by an absorbed power-law model with photon indices of 2.2±0.1 and 1.6±0.2, respectively. The photon indices as well as the flux ratio of F nebula/ F po;.,li" ~ 4 lead us to propose that the system is a pulsar wind nebula, although pulsations have not yet been detected. If we attribute its origin to the Cygnus Loop supernova, then the 0.5- 8 keY luminosity of the nebula is computed to be 2.1xlo"' (d/MOpc)2ergss-" where d is the distance to the Loop. This implies a spin-down loss-energy E ~ 2.6 X 1035 (d/MOpc)2ergss-'. The location of the neutron star candidate, ~2° away from the geometric center of the Loop, implies a high transverse velocity of ~ 1850(8/2D ) (d/540pc) (t/lOkyr)- ' kms-" assuming the currently accepted age of the Cygnus Loop. Subject headings: ISM: individual objects (Cygnus Loop) - ISM: supernova remnants - pulsars: general - stars: neutron - stars: winds, outflows - X-rays: ISM 'RlKEN (The Institute of Physical and Chemical Research), 2-1 Hirosawa, Wako, Sailama 351-0198 2Department of EaTth and Space Science, Graduate School of Science, Osaka University, 1-1 Machikaneyama, Thyonaka, Osaka, 60-0043, Japan SDepartment of Applied Physics, Faculty of Engineering, University of Miyazaki, 1-1 Gakuen Klbana-dai Nishi, Miyazaki, 889-2192, Japan ' Department of PhysiCS, Kyoto University, Kitashirakawa-oiwake-clto, Sakyo, Kyoto 606-8502, J apan 'NASA Goddard Space Flight Center, Code 662, Greenbelt MD 20771 - 2 - 1. -
Survey of Microbial Composition And
The Proceedings of the International Conference on Creationism Volume 7 Article 11 2013 Survey of Microbial Composition and Mechanisms of Living Stromatolites of the Bahamas and Australia: Developing Criteria to Determine the Biogenicity of Fossil Stromatolites Georgia Purdom Answers in Genesis Andrew A. Snelling Answers in Genesis Follow this and additional works at: https://digitalcommons.cedarville.edu/icc_proceedings DigitalCommons@Cedarville provides a publication platform for fully open access journals, which means that all articles are available on the Internet to all users immediately upon publication. However, the opinions and sentiments expressed by the authors of articles published in our journals do not necessarily indicate the endorsement or reflect the views of DigitalCommons@Cedarville, the Centennial Library, or Cedarville University and its employees. The authors are solely responsible for the content of their work. Please address questions to [email protected]. Browse the contents of this volume of The Proceedings of the International Conference on Creationism. Recommended Citation Purdom, Georgia and Snelling, Andrew A. (2013) "Survey of Microbial Composition and Mechanisms of Living Stromatolites of the Bahamas and Australia: Developing Criteria to Determine the Biogenicity of Fossil Stromatolites," The Proceedings of the International Conference on Creationism: Vol. 7 , Article 11. Available at: https://digitalcommons.cedarville.edu/icc_proceedings/vol7/iss1/11 Proceedings of the Seventh International Conference on Creationism. Pittsburgh, PA: Creation Science Fellowship SURVEY OF MICROBIAL COMPOSITION AND MECHANISMS OF LIVING STROMATOLITES OF THE BAHAMAS AND AUSTRALIA: DEVELOPING CRITERIA TO DETERMINE THE BIOGENICITY OF FOSSIL STROMATOLITES Georgia Purdom, PhD, Answers in Genesis, P.O. Box 510, Hebron, KY, 41048 Andrew A. -
The Milesian Calendar in Short
The Milesian calendar in short Quick description The Milesian calendar is a solar calendar, with weighted months, in phase with seasons. It enables you to understand and take control of the Earth’s time. The next picture represents the Milesian calendar with the mean solstices and equinoxes. Leap days The leap day is the last day of the year, it is 31 12m or 12m 31 (whether you use British or American English). This day comes just before a leap year. Years The Milesian years are numbered as the Gregorian ones. However, they begin 10 or 11 days earlier. 1 Firstem Y (1 1m Y) corresponds to 21 December Y-1 when Y is a common year, like 2019. But it falls on 22 December Y-1 when Y is a leap year like 2020. The mapping between Milesian and Gregorian dates is shifted by one for 71 days during “leap winters”, i.e. from 31 Twelfthem to 9 Thirdem. 10 Thirdem always falls on 1 March, and each following Milesian date always falls on a same Gregorian date. Miletus S.A.R.L. – 32 avenue Théophile Gautier – 75016 Paris RCS Paris 750 073 041 – Siret 750 073 041 00014 – APE 7022Z Date conversion with the Gregorian calendar The first day of a Milesian month generally falls on 22 of the preceding Gregorian month, e.g.: 1 Fourthem (1 4m) falls on 22 March, 1 Fifthem (1 5m) on 22 April etc. However: • 1 Tenthem (1 10m) falls on 21 September; • 1 12m falls on 21 November; • 1 1m of year Y falls on 21 December Y-1 if Y is a common year, but on 22 December if Y is a leap year; • 1 2m and 1 3m falls on 21 January and 21 February in leap years, 20 January and 20 February in common years. -
Science Discovery with Diverse Multi-Wavelength Data Fused in NED Joseph Mazzarella Caltech, IPAC/NED
Science Discovery with Diverse Multi-wavelength Data Fused in NED Joseph Mazzarella Caltech, IPAC/NED NED Team: Ben Chan, Tracy Chen, Cren Frayer, George Helou, Scott Terek, Rick Ebert, Tak Lo, Barry Madore, Joe Mazzarella, Olga Pevunova, Marion Schmitz, Ian Steer, Cindy Wang, Xiuqin Wu 7 Oct 2019 ADASS XXIX Groningen 1 Intro & outline Astro data are growing at an unprecedented rate. Ongoing expansion in volume, velocity and variety of data is creating great challenges, and exciting opportunities for discoveries from federated data. Advances in joining data across the spectrum from large sky surveys with > 100,000 smaller catalogs and journal articles, combined with new capabilities of the user interface, are helping astronomers make new discoveries directly from NED. This will be demonstrated with a tour of exciting scientific results recently enabled or facilitated by NED. Some challenges and limitations in joining heterogeneous datasets Outlook for the future 2 Overview: NED is maintaining a panchromatic census of the extragalactic Universe NED is: Published: • Linked to literature • Names • A synthesis of multi- and mission archives • (α,δ) wavelength data • Accessible via VO • Redshifts • D • Published data protocols Mpc • Easy-to-use • Fluxes augmented with • Sizes • Comprehensive derived physical • Attributes attributes • Growing rapidly • References • Notes Contributed: NED simplifies and accelerates • Images NED contains: • Spectra • 773 million multiwavelength cross-IDs scientific research on extragalactic • 667 million distinct objects Derived: • 4.9 billion photometric data points objects by distilling and synthesizing • Distances • 47 million object links to references data across the spectrum, and • Metric sizes SEDs • 7.9 million objects with redshifts providing value-added derived • Luminosities Aλ • 2.5 million images • Velocity corrections • And more .. -
Hubble Revisits the Veil Nebula 2 April 2021
Image: Hubble revisits the Veil Nebula 2 April 2021 this stellar violence, the shockwaves and debris from the supernova sculpted the Veil Nebula's delicate tracery of ionized gas—creating a scene of surprising astronomical beauty. The Veil Nebula is also featured in Hubble's Caldwell Catalog, a collection of astronomical objects that have been imaged by Hubble and are visible to amateur astronomers in the night sky. Provided by NASA Credit: ESA/Hubble & NASA, Z. Levay This image taken by the NASA/ESA Hubble Space Telescope revisits the Veil Nebula, which was featured in a previous Hubble image release. In this image, new processing techniques have been applied, bringing out fine details of the nebula's delicate threads and filaments of ionized gas. To create this colorful image, observations were taken by Hubble's Wide Field Camera 3 instrument using five different filters. The new post-processing methods have further enhanced details of emissions from doubly ionized oxygen (seen here in blues), ionized hydrogen, and ionized nitrogen (seen here in reds). The Veil Nebula lies around 2,100 light-years from Earth in the constellation of Cygnus (the Swan), making it a relatively close neighbor in astronomical terms. Only a small portion of the nebula was captured in this image. The Veil Nebula is the visible portion of the nearby Cygnus Loop, a supernova remnant formed roughly 10,000 years ago by the death of a massive star. That star—which was 20 times the mass of the Sun—lived fast and died young, ending its life in a cataclysmic release of energy. -
Binocular Challenge Here
AHSP Binocular Observing Award Compiled by Phil Harrington www.philharrington.net • To qualify for the BOA pin, you must see 15 of the following 20 binocular targets. Check off each as you spot them. Seen # Object Const. Type* RA Dec Mag Size Nickname 1. M13 Her GC 16 41.7 +36 28 5.9 16' Great Hercules Globular 2. M57 Lyr PN 18 53.6 +33 02 9.7 86"x62" Ring Nebula 3. Collinder 399 Vul AS 19 25.4 +20 11 3.6 60' Coathanger/Brocchi’s Cluster 3.1 4. Albireo Cyg Dbl 19 30.7 +27 57 35” Color Contrasting Double 5.1 5. M27 Vul PN 19 59.6 +22 43 8.1 8’x6’ Dumbbell Nebula 6. NGC 6992 Cyg SNR 20 56.4 +31 43 - 60'x8 Veil Nebula (east) 7. NGC 7000 Cyg BN 20 58.8 +44 20 - 120'x100' North America Nebula 8. M15 Peg GC 21 30.0 +12 10 7.5 12’ Great Pegasus Cluster 9. M39 Cyg OC 21 32.2 +48 26 4.6 32' 10. Barnard 168 Cyg DN 21 53.2 +47 12 - 100'x10' West of Cocoon Nebula 11. IC 5146 Cyg BN/OC 21 53.5 +47 16 - 12'x12' Cocoon Nebula 12. M110 And Gx 00 40.4 +41 41 10 17’x10’ 13. M32 And Gx 00 42.8 +40 52 10 8’x6’ 14. M31 And Gx 00 42.8 +41 16 4.5 178’ Andromeda Galaxy 15. NGC 457 Cas OC 01 19.1 +58 20 6.4 13’ Owl Cluster/ET Cluster 16.