A Laboratory for Binary Evolution
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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 . -
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A&A 536, A27 (2011) Astronomy DOI: 10.1051/0004-6361/201116969 & c ESO 2011 Astrophysics Formation of a disk structure in the symbiotic binary AX Persei during its 2007–10 precursor-type activity A. Skopal1,, T. N. Tarasova2, Z. Cariková1,F.Castellani3, G. Cherini3, S. Dallaporta3, A. Frigo3, C. Marangoni3, S. Moretti3, U. Munari4,G.L.Righetti3,A.Siviero5,S.Tomaselli3, A. Vagnozzi3, and P. Valisa3 1 Astronomical Institute, Slovak Academy of Sciences, 059 60 Tatranská Lomnica, Slovakia 2 Crimean Astrophysical Observatory, Nauchny, Ukraine 3 ANS Collaboration, c/o Osservatorio Astronomico di Padova, Sede di Asiago, 36032 Asiago (VI), Italy 4 INAF Osservatorio Astronomico di Padova, Sede di Asiago, 36032 Asiago (VI), Italy 5 Dipartimento di Astronomia, Universita’ di Padova, Osservatorio Astrofisico, 36012 Asiago (VI), Italy Received 28 March 2011 / Accepted 12 September 2011 ABSTRACT Context. AX Per is an eclipsing symbiotic binary. During active phases, deep narrow minima are observed in its light curve, and the ionization structure in the binary changes significantly. From ∼2007.5, AX Per entered a new active phase. Aims. We aim to derive the ionization structure in the binary and its changes during the recent active phase. Methods. We used optical high- and low-resolution spectroscopy and UBVRCIC photometry. We modeled the SED in the optical and broad wings of the Hα line profile during the 2007–10 higher level of the AX Per activity. Results. After 10 orbital cycles (∼18.6 years), we again measured the eclipse of the hot component by its giant companion in the light curve. We derived a radius of 27 ± 2 R for the eclipsed object and 115 ± 2 R for the eclipsing cool giant. -
The Maunder Minimum and the Variable Sun-Earth Connection
The Maunder Minimum and the Variable Sun-Earth Connection (Front illustration: the Sun without spots, July 27, 1954) By Willie Wei-Hock Soon and Steven H. Yaskell To Soon Gim-Chuan, Chua Chiew-See, Pham Than (Lien+Van’s mother) and Ulla and Anna In Memory of Miriam Fuchs (baba Gil’s mother)---W.H.S. In Memory of Andrew Hoff---S.H.Y. To interrupt His Yellow Plan The Sun does not allow Caprices of the Atmosphere – And even when the Snow Heaves Balls of Specks, like Vicious Boy Directly in His Eye – Does not so much as turn His Head Busy with Majesty – ‘Tis His to stimulate the Earth And magnetize the Sea - And bind Astronomy, in place, Yet Any passing by Would deem Ourselves – the busier As the Minutest Bee That rides – emits a Thunder – A Bomb – to justify Emily Dickinson (poem 224. c. 1862) Since people are by nature poorly equipped to register any but short-term changes, it is not surprising that we fail to notice slower changes in either climate or the sun. John A. Eddy, The New Solar Physics (1977-78) Foreword By E. N. Parker In this time of global warming we are impelled by both the anticipated dire consequences and by scientific curiosity to investigate the factors that drive the climate. Climate has fluctuated strongly and abruptly in the past, with ice ages and interglacial warming as the long term extremes. Historical research in the last decades has shown short term climatic transients to be a frequent occurrence, often imposing disastrous hardship on the afflicted human populations. -
Sky-High 2009
Sky-High 2009 Total Solar Eclipse, 29th March 2006 The 17th annual guide to astronomical phenomena visible from Ireland during the year ahead (naked-eye, binocular and beyond) By John O’Neill and Liam Smyth Published by the Irish Astronomical Society € 5 P.O. Box 2547, Dublin 14, Ireland. e-mail: [email protected] www.irishastrosoc.org Page 1 Foreword Contents 3 Your Night Sky Primer We send greetings to all fellow astronomers and welcome them to this, the seventeenth edition of 5 Sky Diary 2009 Sky-High. 8 Phases of Moon; Sunrise and Sunset in 2009 We thank the following contributors for their 9 The Planets in 2009 articles: Patricia Carroll, John Flannery and James O’Connor. The remaining material was written by 12 Eclipses in 2009 the editors John O’Neill and Liam Smyth. The Gal- 14 Comets in 2009 lery has images and drawings by Society members. The times of sunrise etc. are from SUNRISE by J. 16 Meteors Showers in 2009 O’Neill. 17 Asteroids in 2009 We are always glad to hear what you liked, or 18 Variable Stars in 2009 what you would like to have included in Sky-High. If we have slipped up on any matter of fact, let us 19 A Brief Trip Southwards know. We can put a correction in future issues. And if you have any problem with understanding 20 Deciphering Star Names the contents or would like more information on 22 Epsilon Aurigae – a long period variable any topic, feel free to contact us at the Society e- mail address [email protected]. -
The Abundance of Fluorine in Normal G and K Stars of the Galactic Thin
THE ABUNDANCE OF FLUORINE IN NORMAL G AND K STARS OF THE GALACTIC THIN DISK C. A. Pilachowski1 & Cameron Pace1 Astronomy Department, Indiana University Bloomington, Swain West 319, 727 East Third Street, Bloomington, IN 47405-7105, USA; [email protected], [email protected] ABSTRACT The abundance of fluorine is determined from the (2-0) R9 2.3358 µm fea- ture of the molecule HF for several dozen normal G and K stars in the Galactic thin disk from spectra obtained with the Phoenix IR spectrometer on the 2.1-m telescope at Kitt Peak. The abundances are analyzed in the context of Galactic chemical evolution to explore the contributions of supernovae and asymptotic giant branch (AGB) stars to the abundance of fluorine in the thin disk. The av- erage abundance of fluorine in the thin disk is found to be [F/Fe] = +0.23 ± 0.03, and the [F/Fe] ratio is flat or declines slowly with metallicity in the range from –0.6 < [Fe/H] < +0.3, within the limits of our estimated uncertainty. The mea- sured abundance of fluorine and lack of variation with metallicity in Galactic thin disk stars suggest neutrino spallation in Type II supernovae contributes sig- nificantly to the Galactic fluorine abundance, although contributions from AGB stars may also be important. Subject headings: stars: abundances; stars: late type; Galaxy: abundances; Galaxy: disk arXiv:1507.01550v1 [astro-ph.SR] 6 Jul 2015 Facility: KPNO: 2.1m (Phoenix) 1Visiting Astronomer, Kitt Peak National Observatory. KPNO is operated by AURA, Inc. under contract to the National Science Foundation. -
Arxiv:0908.2624V1 [Astro-Ph.SR] 18 Aug 2009
Astronomy & Astrophysics Review manuscript No. (will be inserted by the editor) Accurate masses and radii of normal stars: Modern results and applications G. Torres · J. Andersen · A. Gim´enez Received: date / Accepted: date Abstract This paper presents and discusses a critical compilation of accurate, fun- damental determinations of stellar masses and radii. We have identified 95 detached binary systems containing 190 stars (94 eclipsing systems, and α Centauri) that satisfy our criterion that the mass and radius of both stars be known to ±3% or better. All are non-interacting systems, so the stars should have evolved as if they were single. This sample more than doubles that of the earlier similar review by Andersen (1991), extends the mass range at both ends and, for the first time, includes an extragalactic binary. In every case, we have examined the original data and recomputed the stellar parameters with a consistent set of assumptions and physical constants. To these we add interstellar reddening, effective temperature, metal abundance, rotational velocity and apsidal motion determinations when available, and we compute a number of other physical parameters, notably luminosity and distance. These accurate physical parameters reveal the effects of stellar evolution with un- precedented clarity, and we discuss the use of the data in observational tests of stellar evolution models in some detail. Earlier findings of significant structural differences between moderately fast-rotating, mildly active stars and single stars, ascribed to the presence of strong magnetic and spot activity, are confirmed beyond doubt. We also show how the best data can be used to test prescriptions for the subtle interplay be- tween convection, diffusion, and other non-classical effects in stellar models. -
The Ephemeris Encyclopedia Galactica: Unexplored Space
The Ephemeris Encyclopedia Galactica: Unexplored Space Sample file 2 Copyright © 2015 Nomadic Delirium Press http://www.nomadicdeliriumpress.com All rights reserved. No part of this book may be reproduced or transmitted in any form or by any means, electronic, mechanical, including photocopying, recording, or by any informational storage and retrieval system, without the written consent of the publisher, except by a reviewer who wishes to quote brief passages in connection with a review written for inclusion in a magazine, newspaper, website, broadcast, etc. Nomadic Delirium Press Aurora, Colorado Sample file 3 INTRODUCTION TO SECTOR FORTY-TWO Welcome to The Ephemeris Encyclopedia Galactica: Sector Forty-Two, an examination of a sector of what is known as “deep space”. The version you are reading is in the Human’s lingua franca. If you are not human, and would like to read it in your species’ native tongue, please consult a data bank on one of your species’ planets and download the appropriate version. Since it’s assumed that you are human, the text in this volume of the Encyclopedia is laid out in a way that will be easy for you to understand. Each star system is listed by the name that your species calls it, and the listings are arranged in order from the closest to your home system out to the ones farthest from your home system. All distances are listed in light years, since that’s what you use on your homeworld. Since this volume of the Encyclopedia is written for humans, it might be safe to assume that you already know all of the details of these systems, but just in case, we’re including everything we can here. -
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. -
X. Bayesian Stellar Parameters and Evolutionary Stages for 372 Giant Stars from the Lick Planet Search?
A&A 616, A33 (2018) Astronomy https://doi.org/10.1051/0004-6361/201833111 & c ESO 2018 Astrophysics Precise radial velocities of giant stars X. Bayesian stellar parameters and evolutionary stages for 372 giant stars from the Lick planet search? Stephan Stock, Sabine Reffert, and Andreas Quirrenbach Landessternwarte, Zentrum für Astronomie der Universität Heidelberg, Königstuhl 12, 69117 Heidelberg, Germany e-mail: [email protected] Received 27 March 2018 / Accepted 4 May 2018 ABSTRACT Context. The determination of accurate stellar parameters of giant stars is essential for our understanding of such stars in general and as exoplanet host stars in particular. Precise stellar masses are vital for determining the lower mass limit of potential substellar companions with the radial velocity method, but also for dynamical modeling of multiplanetary systems and the analysis of planetary evolution. Aims. Our goal is to determine stellar parameters, including mass, radius, age, surface gravity, effective temperature and luminosity, for the sample of giants observed by the Lick planet search. Furthermore, we want to derive the probability of these stars being on the horizontal branch (HB) or red giant branch (RGB), respectively. Methods. We compare spectroscopic, photometric and astrometric observables to grids of stellar evolutionary models using Bayesian inference. Results. We provide tables of stellar parameters, probabilities for the current post-main sequence evolutionary stage, and probability density functions for 372 giants from the Lick planet search. We find that 81% of the stars in our sample are more probably on the HB. In particular, this is the case for 15 of the 16 planet host stars in the sample. -
Switching on the First Light in the Universe
Ludwig-Maximilians-Universit¨at Sigillum Universitatis Ludovici Maximiliani Switching on the first light in the Universe Dissertation der Fakult¨at f¨ur Physik Dissertation of the Faculty of Physics / Dissertazione della Facolta` di Fisica der Ludwig-Maximilians-Universit¨at M¨unchen at the Ludwig Maximilian University of Munich / dell’Universita` Ludwig Maximilian di Monaco f¨ur den Grad des for the degree of / per il titolo di Doctor rerum naturalium vorgelegt von Umberto Maio presented by / presentata da aus Montella, AV (Italy) from / da M¨unchen, 10.10.2008 Sigillum Universitatis Ludovici Maximiliani 1. Gutachter: Prof. Dr. Simon D. M. White referee: / relatore: 2. Gutachter: Prof. Dr. Andreas M. Burkert referee: / relatore: Tag der m¨undlichen Pr¨ufung: 12.12.2008 Date of the oral exam: / Data dell’esame orale: Curriculum vitæ et studiorum Umberto Maio Personal data First Name: Umberto Last name: Maio Date of birth: 22nd March, 1981 Place of birth: Avellino (Italy) Citizenship: Italian Hobbies: Literature, History, Philosophy, reading Sports: swimming, playing footbal, cycling, running Languages: Italian, English, German, Latin Contacts B Address: c/o Max-Planck-Institut f¨ur Astrophysik Karl-Schwarzschild-Straße, 1 D-85748 Garching b. M¨unchen - M (Germany) or via della Libera, 25 83048 Montella, AV (Italy) Phone: +49 (0)89 30 000 2196, +39 (0)827 61275 H Mobile: +49 (0)176 4714638, +39 (0)328 3826882 @ E-mail: [email protected], [email protected] Education 2008, 12th December: Ph. D. rer. nat. Ludwig-Maximilians-Universit¨at M¨unchen Max-Planck-Institut f¨ur Astrophysik (Garching b. M¨unchen) 2005, 14th July: Laurea in Astronomy, University of Bologna Alma Mater Studiorum (Italy) Faculty of Mathematical,· Physical and Natural Sciences Department of Astronomy Thesis: Early structure formation in quintessence models Supervisor: Prof. -
ARDEN VUL TABLE of CONTENTS General Introduction a Brief History of Arden Vul
ARDEN VUL TABLE OF CONTENTS General Introduction A Brief History of Arden Vul ..................................................V. 1 P. 7 Sub-Level 1: The Tombs of Light ...........................................V. 3 P. 3 Design Principles ...................................................................V. 1 P. 10 Sub-Level 2: The Hall of Shrines ..........................................V. 3 P. 11 Note on Designation of Keyed Locations ...........................V. 1 P. 11 Sub-Level 3: The Lesser Baboon Caves ...............................V. 3 P. 23 Starting Levels for PCs ..........................................................V. 1 P. 11 Sub-Level 4: The Goblin Warrens........................................ V. 3 P. 33 General Construction Features ...........................................V. 1 P. 12 Sub-Level 5: The Lizardman Caves .....................................V. 3 P. 57 Iconic Locations of Arden Vul .............................................V. 1 P. 14 Sub-Level 6: The Drowned Canyon ....................................V. 3 P. 73 Rumors ....................................................................................V. 1 P. 18 Sub-Level 7: The Flooded Vaults .......................................V. 3 P. 117 Factions of Arden Vul ...........................................................V. 1 P. 30 Sub-Level 8: The Caves Behind the Falls ..........................V. 3 P. 125 Adventure Hooks ...................................................................V. 1 P. 48 Sub-Level 9: The Kaliyani Pits ...........................................V. -
Venus and Mercury Are Back
FORT WORTH ASTRONOMICAL SOCIETY (est. 1949) NOVEMBER 2011 Venus and Mercury Are Back In This Issue November Club Calendar ... 2 Night Sky Chart ... 3 Cloudy Night Library ... 4 The Gray Cubicle You Want To Work In ... 6 Clues From Ancient Light ... 7 This Month’s Constellation - Pisces ... 8 Image courtesy of science.nasa.gov PRIME FOCUS - FORT WORTH ASTRONOMICAL SOCIETY NOVEMBER 2011 November 2011 Sun Mon Tue Wed Thu Fri Sat 1 2 3 4 5 1st Quarter Moon 11:38pm 6 7 8 9 10 11 12 Day Light Saving Asteroid 2005 Neptune is Full Moon Veterans Day ends at 2am YU55 passes only stationary 2:16pm 202,000mi from Earth 13 14 15 16 17 18 19 Leonid meteor Last Quarter shower peaks Moon 9:09am FWAS Monthly Meeting 20 21 22 23 24 25 26 Thanksgiving Day New Moon 12:10am Mercury is stationary 27 28 29 30 2 PRIME FOCUS - FORT WORTH ASTRONOMICAL SOCIETY NOVEMBER 2011 November Night Sky November 15, 2011 @ 10:00pm CST Sky chart coutesy of Chris Peat and http://www.heavens-above.com/ Planet Viewing This Month Mercury is in the western evening sky and remains about 20 from Venus for the first half of the month. Venus sits low in the southwestern evening twilight. Mars is mostly out of the picture but can be spotted in Leo early in the morning. Jupiter has just passed opposition and still traverses the sky all evening, setting near dawn. Although the angle of ecliptic favors the Northern Hemisphere, Saturn can be seen in the pre-dawn sky, in Virgo.