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The Pennsylvania State University The Graduate School Department of Astronomy and Astrophysics THE VIEW THROUGH THE WIND: X-RAY OBSERVATIONS OF BROAD ABSORPTION LINE QUASI-STELLAR OBJECTS A Thesis in Astronomy and Astrophysics by Sarah Connoran Gallagher c 2002 Sarah Connoran Gallagher Submitted in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy May 2002 We approve the thesis of Sarah Connoran Gallagher. Date of Signature W. Nielsen Brandt Associate Professor of Astronomy and Astrophysics Thesis Adviser Chair of Committee Jane C. Charlton Associate Professor of Astronomy and Astrophysics Michael C. Eracleous Assistant Professor of Astronomy and Astrophysics L. Samuel Finn Associate Professor of Physics Gordon P. Garmire Evan Pugh Professor of Astronomy and Astrophysics Steinn Sigurdsson Assistant Professor of Astronomy and Astrophysics Peter I. M´esz´aros Professor of Astronomy and Astrophysics Head of the Department of Astronomy and Astrophysics iii Abstract The 2{10 keV bandpasses and unprecedented sensitivity of modern X-ray obser- vatories have enabled new insights into the immediate environments of Broad Absorp- tion Line (BAL) QSOs. BAL QSOs, approximately 10% of the QSO population, exhibit deep, broad absorption lines from high ionization ultraviolet resonance transitions. These blueshifted absorption features are understood to arise along lines of sight which travel through radiatively driven winds with terminal velocities reaching 0.1{0:3c. These en- ergetic outflows are an important component of QSO environments; mass ejection is apparently fundamentally linked to the process of active mass accretion onto super- massive black holes. X-rays, generated in the innermost regions surrounding accreting black holes, travel through the nuclear environments to the observer. -
Diamonds in the Sky
Diamonds in the Sky Edited by Mike Brotherton.PhD. Contents In the Autumn of Empire (Jerry Oltion) A cautionary tale about why scientific misconceptions can be important. This story will also be appearing in Analog soon. Keywords: The seasons. Misconceptions. End of the World (Alma Alexander) Nothing is forever, not even the earth and sky. Keywords: Evolution of the sun. The Freshmen Hookup (Wil McCarthy) An exploration of how the elements are built in stars using the antics of college freshmen as a metaphor. Keywords: Stellar nucleosynthesis. Galactic Stress (David Levine) You think your life is stressful? How about having to deal with the entire universe? Keywords: Scales of the Universe. The Moon is a Harsh Pig (Gerald M. Weinberg) Robert Heinlein's novel The Moon is a Harsh Mistress about a revolt on the Moon was a landmark novel of the 1960s. Jerry's story is also educational. Keywords: Phases of the Moon, Misconceptions. The Point (Mike Brotherton) What is the meaning of life in an expanding universe? This story previously appeared at http://www.mikebrotherton.com. Keywords: Cosmology. Squish (Dan Hoyt) How would you like a whirlwind tour of the planets? Keywords: The Solar System. Jaiden's Weaver (Mary Robinette Kowal) So many things about life on Earth depend on the cycles of the sky, from the moon and tides to seasons and more. Well, what if the sky were different? How would humans adapt to life on a world with rings? Keywords: Planetary rings. How I Saved the World (Valentin Ivanov) The movies Armageddon and Deep Impact featured nuclear bombs to divert asteroids headed for Earth, but this is really not the best way to deal with this threat. -
THE BINARY BLACK HOLE MODEL for MRK 231 BITES the DUST Karen M
The Astrophysical Journal, 829:4 (17pp), 2016 September 20 doi:10.3847/0004-637X/829/1/4 © 2016. The American Astronomical Society. All rights reserved. THE BINARY BLACK HOLE MODEL FOR MRK 231 BITES THE DUST Karen M. Leighly1,5, Donald M. Terndrup2, Sarah C. Gallagher3, and Adrian B. Lucy4 1 Homer L. Dodge Department of Physics and Astronomy, The University of Oklahoma, 440 W. Brooks Street, Norman, OK 73019, USA 2 Department of Astronomy, The Ohio State University, 140 W. 18th Avenue, Columbus, OH 43210, USA 3 Department of Physics & Astronomy and Centre for Planetary and Space Exploration, The University of Western Ontario, London, ON N6A 3K7, Canada 4 Department of Astronomy, Columbia University, 550 W. 120th Street, New York, NY 10027, USA Received 2016 April 12; revised 2016 July 7; accepted 2016 July 8; published 2016 September 13 ABSTRACT Mrk231 is a nearby quasar with an unusually red near-UV-to-optical continuum, generally explained as heavy reddening by dust. Yan et al. proposed that Mrk231 is a milliparsec black hole binary with little intrinsic reddening. We show that if the observed FUV continuum is intrinsic, as assumed by Yan et al., it fails by a factor of about 100 in powering the observed strength of the near-infrared emission lines and the thermal near and mid- infrared continuum. In contrast, the line and continuum strengths are typical for a reddened AGN spectral energy * distribution (SED).Wefind that the He I /Pβ ratio is sensitive to the SED for a one-zone model. If this sensitivity is maintained in general broadline region models, then this ratio may prove a useful diagnostic for heavily reddened quasars. -
Sabrina Lyn Cales
Sabrina Lyn Cales Yale Center for Astronomy and Astrophysics Physics Department Yale University New Haven, CT 06520-8120 Phone: (203) 436-4951 Fax: (203) 432-3824 E-Mail: [email protected] Current Position Yale University: Joint Yale University - Universidad de Concepcion ALMA 2014-Current Postdoctoral Fellow Project: Caught in a Cosmic Tango: ALMA Spies the Interplay Between Dual AGN in Merger Remnant Galaxies Mentors: Meg Urry, Ezequiel Treister Education Ph.D. Physics, University of Wyoming August 2012 Thesis: Understanding Post-starburst Quasars Advisor: Professor Mike Brotherton M.S. Physics, University of Wyoming May 2011 B.A. Physics with Math Minor, University of California at June 2005 Riverside Thesis: Luminosity Distribution for Broad Absorption Line QSOs Advisor: Gabriela Canalizo Science Interests AGN environments, AGN host galaxies, Merger driven black hole and galaxy growth, Stochastic black hole accretion Honors and Awards Joint Yale University – Universidad de Concepcion ALMA 2012-2015 Postdoctoral Fellowship NSF GK-12 Graduate Education Fellowship, $60,000 2007-2008, 2011-2012 NASA Earth and Space Science Fellowship, $90,000 2008-2011 Summer Research Experience for Winston-Salem State University 2011 Students, Mentor, $2,500 Dean’s Fellow Summer Internship, University of California at 2004 Riverside, $3,000 Publications and Talks • Three papers as main author in refereed journals, two papers submitted, two manuscripts. • Fourteen papers in refereed journals, three papers submitted to MNRAS, one paper submitted -
Measuring and Extrapolating the Chemical Abundances of Normal and Superluminous Core-Collapse Supernovae
Measuring and Extrapolating the Chemical Abundances of Normal and Superluminous Core-Collapse Supernovae Dissertation Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the Graduate School of The Ohio State University By Rebecca A. Stoll Graduate Program in Astronomy The Ohio State University 2013 Dissertation Committee: Professor Richard W. Pogge, Advisor Professor Paul Martini Professor Todd A. Thompson Copyright by Rebecca A. Stoll 2013 Abstract We present All-Sky Automated Survey data starting 25 days before the discovery of the recent type IIn SN 2010jl, and we compare its light curve to other luminous IIn SNe, showing that it is a luminous (MI 20.5) event. Its host galaxy, ≈ − UGC 5189, has a low gas-phase oxygen abundance (12+log(O/H) = 8.2 0.1), which ± reinforces the emerging trend that over-luminous core-collapse supernovae are found in the low-metallicity tail of the galaxy distribution, similar to the known trend for the hosts of long GRBs. We compile oxygen abundances from the literature and from our own observations of UGC 5189, and we present an unpublished spectrum of the luminous type Ic SN 2010gx that we use to estimate its host metallicity. We discuss these in the context of host metallicity trends for different classes of core-collapse objects. The earliest generations of stars are known to be enhanced in [O/Fe] relative to the Solar mixture; it is therefore likely that the stellar progenitors of these overluminous supernovae are even more iron-poor than they are oxygen-poor. A number of mechanisms and massive star progenitor systems have been proposed to explain the most luminous core-collapse supernovae. -
Curriculum Vitae — Patrick Brian Hall Professor, York University December 16, 2020
Curriculum Vitae — Patrick Brian Hall Professor, York University December 16, 2020 Office address: Petrie 337, 416-736-2100 x77752, FAX 416-736-5516, [email protected] Mailing address: Department of Physics & Astronomy, York University, 4700 Keele St., Toronto, ON M3J 1P3, Canada Degrees • Ph.D. Astronomy, University of Arizona, Dept. of Astronomy, January 1998 Thesis: An Optical/Infrared Study of Radio-Loud Quasar Environments Advisor: Dr. Richard F. Green • B.A. Astronomy, University of California at Berkeley, Dept. of Astronomy, May 1990 • B.A. Physics, University of California at Berkeley, Dept. of Physics, May 1990 Employment History 07/20-present Chair and Biophysics Program Coordinator, Department of Physics and Astronomy, York University 07/16-present Professor and Member of the Faculty of Graduate Studies, Department of Physics and Astronomy, York University 07/14-06/17, 07/19-06/20 Undergraduate Program Director, Dept. of Physics and Astronomy, York University 07/09-06/16 Associate Professor and Member of the Faculty of Graduate Studies, Department of Physics and Astronomy, York University 07/04-06/09 Assistant Professor and Member of the Faculty of Graduate Studies, Department of Physics and Astronomy, York University 10/03-06/04 Research Associate, Department of Astrophysical Sciences, Princeton University 10/00-9/03 Research Associate, Princeton University Observatory, Princeton University; and Investigador Asociado, Depto. de Astronom´ıa, P. Universidad Catolica´ de Chile 1/98-9/00 Post-Doctoral Fellow, Department of Astronomy,