Observer's Handbook 1969
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Publications Et Communications De Florentin Millour (Février 2016) H-Index 21, Total : 130 Publications Dont 53 À Comité De Lecture
Publications et communications de Florentin Millour (Février 2016) h-index 21, total : 130 publications dont 53 à comité de lecture. Articles dans des revues à comité de lecture, thèse 2015 1. Mourard, D., ..., Millour, F. ; et al., . (2015, A&A, 577, 51) Spectral and spatial imaging of the Be+sdO binary Phi Persei 2014 2. Chesneau, O. ; Millour, F. ; de Marco, O. et al., . (2014, A&A, 569, 3) V838 Monocerotis : the central star and its environment a decade after outburst 3. Chesneau, O. ; Millour, F. ; de Marco, O. et al., . (2014, A&A, 569, 4) The RCB star V854 Centauri is surrounded by a hot dusty shell 4. Chesneau, O. ; Meilland, A. ; Chapellier, E. ; Millour, F. ; et al., . (2014, A&A, 563, A71) The yellow hypergiant HR 5171 A : Resolving a massive interacting binary in the common envelope phase. 5. Domiciano de Souza, A. ; Kervella, P. ; Moser Faes, D. et al. (2014, A&A, 569, 10) The environment of the fast rotating star Achernar. III. Photospheric parameters revealed by the VLTI 6. Hadjara, M. ; Domiciano de Souza, A. ; Vakili, F. et al. (2014, A&A, 569, 45) Beyond the diraction limit of optical/IR interferometers. II. Stellar parameters of rotating stars from dierential phases 7. Schutz, A. ; Vannier, M. ; Mary, D. et al. (2014, A&A, 565, 88) Statistical characterisation of polychromatic absolute and dierential squared visibilities obtained from AMBER/VLTI instrument 2013 8. Millour, F. ; Meilland, A. ; Stee, P. & Chesneau, O. (2013, LNP, 857, 149) Interactions in Massive Binary Stars as Seen by Interferometry 9. Stee, P. ; Meilland, A. -
FY13 High-Level Deliverables
National Optical Astronomy Observatory Fiscal Year Annual Report for FY 2013 (1 October 2012 – 30 September 2013) Submitted to the National Science Foundation Pursuant to Cooperative Support Agreement No. AST-0950945 13 December 2013 Revised 18 September 2014 Contents NOAO MISSION PROFILE .................................................................................................... 1 1 EXECUTIVE SUMMARY ................................................................................................ 2 2 NOAO ACCOMPLISHMENTS ....................................................................................... 4 2.1 Achievements ..................................................................................................... 4 2.2 Status of Vision and Goals ................................................................................. 5 2.2.1 Status of FY13 High-Level Deliverables ............................................ 5 2.2.2 FY13 Planned vs. Actual Spending and Revenues .............................. 8 2.3 Challenges and Their Impacts ............................................................................ 9 3 SCIENTIFIC ACTIVITIES AND FINDINGS .............................................................. 11 3.1 Cerro Tololo Inter-American Observatory ....................................................... 11 3.2 Kitt Peak National Observatory ....................................................................... 14 3.3 Gemini Observatory ........................................................................................ -
Double and Multiple Star Measurements in the Northern Sky with a 10” Newtonian and a Fast CCD Camera in 2006 Through 2009
Vol. 6 No. 3 July 1, 2010 Journal of Double Star Observations Page 180 Double and Multiple Star Measurements in the Northern Sky with a 10” Newtonian and a Fast CCD Camera in 2006 through 2009 Rainer Anton Altenholz/Kiel, Germany e-mail: rainer.anton”at”ki.comcity.de Abstract: Using a 10” Newtonian and a fast CCD camera, recordings of double and multiple stars were made at high frame rates with a notebook computer. From superpositions of “lucky images”, measurements of 139 systems were obtained and compared with literature data. B/w and color images of some noteworthy systems are also presented. mented double stars, as will be described in the next Introduction section. Generally, I used a red filter to cope with By using the technique of “lucky imaging”, seeing chromatic aberration of the Barlow lens, as well as to effects can strongly be reduced, and not only the reso- reduce the atmospheric spectrum. For systems with lution of a given telescope can be pushed to its limits, pronounced color contrast, I also made recordings but also the accuracy of position measurements can be with near-IR, green and blue filters in order to pro- better than this by about one order of magnitude. This duce composite images. This setup was the same as I has already been demonstrated in earlier papers in used with telescopes under the southern sky, and as I this journal [1-3]. Standard deviations of separation have described previously [1-3]. Exposure times varied measurements of less than +/- 0.05 msec were rou- between 0.5 msec and 100 msec, depending on the tinely obtained with telescopes of 40 or 50 cm aper- star brightness, and on the seeing. -
Gum 48D: an Evolved HII Region with Ongoing Star Formation
Gum 48d: an evolved HII region with ongoing star formation J.L. Karr Academia Sinica Institute of Astronomy and Astrophysics, Taipei, Taiwan, ROC P. Manoj Department of Physics and Astronomy, University of Rochester, NY N. Ohashi Academia Sinica Institute of Astronomy and Astrophysics, Taipei, Taiwan, ROC ABSTRACT High mass star formation and the evolution of HII regions have a substantial impact on the morphology and star formation history of molecular clouds. The HII region Gum 48d, located in the Centaurus Arm at a distance of 3.5 kpc, is an old, well evolved HII region whose ionizing stars have moved off the main sequence. As such, it represents a phase in the evolution of HII regions that is less well studied than the earlier, more energetic, main sequence phase. In this paper we use multi-wavelength archive data from a variety of sources to perform a detailed study of this interesting region. Morphologically, Gum 48d displays a ring-like faint HII region associated with diffuse emission from the associated PDR, and is formed from part of a large, massive molecular cloud complex. There is extensive ongoing star formation in the region, at scales ranging from low to high mass, which is consistent with triggered star formation scenarios. We investigate the dynamical history and evolution of this region, and conclude that arXiv:0903.0934v1 [astro-ph.GA] 5 Mar 2009 the original HII region was once larger and more energetic than the faint region currently seen. The proposed history of this molecular cloud complex is one of multiple, linked generations of star formation, over a period of 10 Myr. -
508-764-2554 Like to Embrace Rather Than Avoid
PROUD MEDIA SPONSOR OF SOUTHBRIDGE AREA RELAY FOR LIFE! SERVING OUR READERS SINCE 1923 WEDNESDAY , M AY 13, 2009 (508) 764-4325/VISIT US AT: www.theheartofmassachusetts.com Newsstand: 60 cents TODAY’S QUOTE A busy June ballot CANDIDATES FOR COUNCIL HEAD LIST “My closest relation 10 BY GUS STEEVES is myself.” NEWS STAFF WRITER SOUTHBRIDGE — For the — Terence last several elections, Southbridge has bucked the tendency of local races to be TOMORROW’S fairly humdrum. This year T ’ is no exception. WEATHER In fact, the June 30 ballot promises to be the most crowded in recent years. Ten people are running for three seats on the Town Council, five for two school committee seats, and two for town clerk. While many names on the list are repeat candidates, there are several new faces. “This is the first [annual election] where pretty much everybody who pulled out papers returned them,” said Showers Town Clerk Madaline High 64 Daoust. “Maybe we’ll get a Low 53 lot more people to come out VFW AWARDS NIGHT to vote.” In fact, just one person, INNING Shawn Kelley photo W INNING who took out papers for Bay all the candidates last night File photo LOTTERY SOUTHBRIDGE — VFW Man of the Year — Southbridge Police Path School Committee, did in an effort to sample the dif- Poll workers go over absentee bal- Chief Daniel Charette — sits with his wife, Kathleen, and son not return them, leaving that ferent views at issue this lots at West Street School to veri- NUMBERS Jacob, 12, at the group’s 63rd annual testimonial banquet seat without a candidate. -
Black Hole Math Is Designed to Be Used As a Supplement for Teaching Mathematical Topics
National Aeronautics and Space Administration andSpace Aeronautics National ole M a th B lack H i This collection of activities, updated in February, 2019, is based on a weekly series of space science problems distributed to thousands of teachers during the 2004-2013 school years. They were intended as supplementary problems for students looking for additional challenges in the math and physical science curriculum in grades 10 through 12. The problems are designed to be ‘one-pagers’ consisting of a Student Page, and Teacher’s Answer Key. This compact form was deemed very popular by participating teachers. The topic for this collection is Black Holes, which is a very popular, and mysterious subject among students hearing about astronomy. Students have endless questions about these exciting and exotic objects as many of you may realize! Amazingly enough, many aspects of black holes can be understood by using simple algebra and pre-algebra mathematical skills. This booklet fills the gap by presenting black hole concepts in their simplest mathematical form. General Approach: The activities are organized according to progressive difficulty in mathematics. Students need to be familiar with scientific notation, and it is assumed that they can perform simple algebraic computations involving exponentiation, square-roots, and have some facility with calculators. The assumed level is that of Grade 10-12 Algebra II, although some problems can be worked by Algebra I students. Some of the issues of energy, force, space and time may be appropriate for students taking high school Physics. For more weekly classroom activities about astronomy and space visit the NASA website, http://spacemath.gsfc.nasa.gov Add your email address to our mailing list by contacting Dr. -
Primary Velocity and Orbital Phase Effects on Planetary Detectability from Small Epoch Number Data Sets
The Astronomical Journal, 162:26 (16pp), 2021 July https://doi.org/10.3847/1538-3881/abf7b9 © 2021. The Author(s). Published by the American Astronomical Society. Primary Velocity and Orbital Phase Effects on Planetary Detectability from Small Epoch Number Data Sets Cam Buzard1 , Stefan Pelletier2 , Danielle Piskorz3 , Björn Benneke2 , and Geoffrey A. Blake1,3 1 Division of Chemistry and Chemical Engineering, California Institute of Technology, Pasadena, CA 91125, USA; [email protected] 2 Institute for Research on Exoplanets, Université de Montréal, Montreal, QC, Canada 3 Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA Received 2021 January 21; revised 2021 April 2; accepted 2021 April 12; published 2021 June 22 Abstract Cross-correlation analyses of high-resolution spectroscopic data have recently shown great success in directly detecting planetary signals and enabling the characterization of their atmospheres. One such technique aims to observe a system at multiple epochs and combine the measured planetary radial velocities from each epoch into a measurement of the planetary Keplerian orbital velocity Kp, constituting a direct detection of the planetary signal. Recent work has shown that in few-epoch (∼5) data sets, unintended structure can arise at a high level, obscuring the planetary detection. In this work, we look to simulations to examine whether there are ways to reduce this structured noise in few-epoch data sets by careful planning of observations. The choice of observation date allows observers to select the primary (stellar) velocity through a set systemic velocity and chosen barycentric velocity and the planetary orbital phase so we focus on the effects of these two parameters. -
PROJECT ORI'on a Design Study of a System for Detecting Extrasolar Planets
PROJECT ORI'ON A Design Study of a System for Detecting Extrasolar Planets . NASA NASA SP-436 PROJECT ORION A Design Stud? of a System for Detecting Extrasolar Planets David C.Black, Editor Arnes Research Center Nat~cnalAeroriautics and Space Adminislrat~on Scientific and Technical Information Branch 1986) Cover: Orion Nebula XI1 Photograph courtesy of Lick Observatory. Ode to Apodization Twinkle, twinkle, little star Thirty parsecs from where we are. Does your wobble through the sky Mean a planet is nearby? Or has the result come into being Because of one arcsecond seeing? -Raymond P. Vito Library of Congress Cataloging in Publication Data Main entry under title: Project Orion. (NASA SP ; 436) Bibliography: p. 1. Project Orion. I. Black, David C. 11. Series: United States. National Aeronautics and Space Administration. NASA SP ;436. QB602.9.P76 523.1'13 80-11728 For sale by the Sul~erintenclentof Documents. U.S. Gorevnmc~ntPrinting Olficc \X7a\hinrrton n C 70402 TABLE OF CONTENTS Page PREFACE ......................................... ix 1 . INTRODUCTION ................................. 1 Discovery of Our Planetary System .................. 1 Efforts .to Detect Other Planetary Systems ............. 4 Project Orion ................................... 6 2 . TOWARD DESIGN CONCEPTS ..................... 11 Remarks Concerning the Term "Planet" .............. II Detection Problem .Astrophysical Aspects ........... 12 Detectioil Problem .Terrestrial Aspects .............. 24 Detection Problem .Hardware Aspects ............... 30 Summary ..................................... -