Informacja

Drogi użytkowniku, aplikacja do prawidłowego działania wymaga obsługi JavaScript. Proszę włącz obsługę JavaScript w Twojej przeglądarce.

Przeglądasz jako GOŚĆ

Wyszukujesz frazę ""Chomiuk, Laura"" wg kryterium: Autor


Tytuł :
THE RADIO LIGHT CURVE OF THE GAMMA-RAY NOVA IN V407 CYG: THERMAL EMISSION FROM THE IONIZED SYMBIOTIC ENVELOPE, DEVOURED FROM WITHIN BY THE NOVA BLAST.
Autorzy :
Chomiuk, Laura chomiuk@pa.msu.edu
Krauss, Miriam I.
Rupen, Michael P.
Nelson, Thomas
Roy, Nirupam
Sokoloski, Jennifer L.
Mukai, Koji
Munari, Ulisse
Mioduszewski, Amy
Weston, Jennifer
O'Brien, Tim J.
Eyres, Stewart P. S.
Bode, Michael F.
Pokaż więcej
Źródło :
Astrophysical Journal. 12/20/2012, Vol. 761 Issue 2, p1-1. 1p.
Czasopismo naukowe
Tytuł :
MULTI-WAVELENGTH OBSERVATIONS OF SUPERNOVA 2011ei: TIME-DEPENDENT CLASSIFICATION OF TYPE IIb AND Ib SUPERNOVAE AND IMPLICATIONS FOR THEIR PROGENITORS.
Autorzy :
MILISAVLJEVIC, DAN
MARGUTTI, RAFFAELLA
SODERBERG, ALICIA M.
PIGNATA, GIULIANO
CHOMIUK, LAURA
FESEN, ROBERT A.
BUFANO, FILOMENA
SANDERS, NATHAN E.
PARRENT, JEROD T.
PARKER, STUART
MAZZALI, PAOLO
PIAN, ELENA
PICKERING, TIMOTHY
BUCKLEY, DAVID A. H.
CRAWFORD, STEVEN M.
GULBIS, AMANDA A. S.
HETTLAGE, CHRISTIAN
HOOPER, ERIC
NORDSIECK, KENNETH H.
O'DONOGHUE, DARRAGH
Pokaż więcej
Źródło :
Astrophysical Journal. 4/10/2013, Vol. 767 Issue 1, p1-19. 19p.
Czasopismo naukowe
Tytuł :
Binary orbits as the driver of γ-ray emission and mass ejection in classical novae.
Autorzy :
Chomiuk L; Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA.
Linford JD; Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA.
Yang J; 1] Department of Earth and Space Sciences, Chalmers University of Technology, Onsala Space Observatory, SE-439 92 Onsala, Sweden [2] Joint Institute for VLBI in Europe, Postbus 2, NL-7990 AA Dwingeloo, The Netherlands [3] Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, 200030 Shanghai, China.
O'Brien TJ; Jodrell Bank Centre for Astrophysics, Alan Turing Building, University of Manchester, Manchester M13 9PL, UK.
Paragi Z; Joint Institute for VLBI in Europe, Postbus 2, NL-7990 AA Dwingeloo, The Netherlands.
Mioduszewski AJ; National Radio Astronomy Observatory, PO Box O, Socorro, New Mexico 87801, USA.
Beswick RJ; Jodrell Bank Centre for Astrophysics, Alan Turing Building, University of Manchester, Manchester M13 9PL, UK.
Cheung CC; Space Science Division, Naval Research Laboratory, Washington, DC 20375-5352, USA.
Mukai K; 1] Department of Physics, University of Maryland, Baltimore County, 1000 Hilltop Circle, Baltimore, Maryland 21250, USA [2] CRESST and X-ray Astrophysics Laboratory, NASA/GSFC, Greenbelt, Maryland 20771, USA.
Nelson T; School of Physics and Astronomy, University of Minnesota, 115 Church Street Southeast, Minneapolis, Minnesota 55455, USA.
Ribeiro VA; Astrophysics, Cosmology and Gravity Centre, Department of Astronomy, University of Cape Town, Private Bag X3, Rondebosch 7701, South Africa.
Rupen MP; 1] National Radio Astronomy Observatory, PO Box O, Socorro, New Mexico 87801, USA [2] National Research Council, Herzberg Astronomy and Astrophysics, 717 White Lake Road, PO Box 248, Penticton, British Columbia V2A 6J9, Canada.
Sokoloski JL; Columbia Astrophysics Laboratory, Columbia University, New York, New York 10027, USA.
Weston J; Columbia Astrophysics Laboratory, Columbia University, New York, New York 10027, USA.
Zheng Y; Columbia Astrophysics Laboratory, Columbia University, New York, New York 10027, USA.
Bode MF; Astrophysics Research Institute, Liverpool John Moores University, IC2, Liverpool Science Park, 146 Brownlow Hill, Liverpool L3 5RF, UK.
Eyres S; Jeremiah Horrocks Institute for Mathematics, Physics and Astronomy, University of Central Lancashire, Preston PR1 2HE, UK.
Roy N; Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany.
Taylor GB; Department of Physics and Astronomy, University of New Mexico, MSC07 4220, Albuquerque, New Mexico 87131-0001, USA.
Pokaż więcej
Źródło :
Nature [Nature] 2014 Oct 16; Vol. 514 (7522), pp. 339-42. Date of Electronic Publication: 2014 Oct 08.
Typ publikacji :
Journal Article; Research Support, Non-U.S. Gov't; Research Support, U.S. Gov't, Non-P.H.S.
Czasopismo naukowe
Tytuł :
RADIO OBSERVATIONS REVEAL A SMOOTH CIRCUMSTELLAR ENVIRONMENT AROUND THE EXTRAORDINARY TYPE Ib SUPERNOVA 2012au.
Autorzy :
Kamble, Atish
Soderberg, Alicia M.
Chomiuk, Laura
Margutti, Raffaella
Medvedev, Mikhail
Milisavljevic, Dan
Chakraborti, Sayan
Chevalier, Roger
Chugai, Nikolai
Dittmann, Jason
Drout, Maria
Fransson, Claes
Nakar, Ehud
Sanders, Nathan
Pokaż więcej
Źródło :
Astrophysical Journal. 12/10/2014, Vol. 797 Issue 1, p1-1. 1p.
Czasopismo naukowe
Tytuł :
Limits on thermal variations in a dozen quiescent neutron stars over a decade.
Autorzy :
Bahramian, Arash
Heinke, Craig O.
Degenaar, Nathalie
Chomiuk, Laura
Wijnands, Rudy
Strader, Jay
Ho, Wynn C. G.
Pooley, David
Pokaż więcej
Temat :
NEUTRON stars
ACCRETION disks
GLOBULAR clusters
X-ray binaries
STELLAR mass
THERMAL analysis
Źródło :
Monthly Notices of the Royal Astronomical Society; 10/1/2015, Vol. 452 Issue 4, p3475-3488, 14p
Czasopismo naukowe
Tytuł :
Non-thermal radio emission from colliding flows in classical nova V1723 Aql.
Autorzy :
Weston, Jennifer H. S.
Sokoloski, J. L.
Metzger, Brian D.
Yong Zheng
Chomiuk, Laura
Krauss, Miriam I.
Linford, Justin D.
Nelson, Thomas
Mioduszewski, Amy J.
Rupen, Michael P.
Finzell, Tom
Mukai, Koji
Pokaż więcej
Temat :
NOVAE (Astronomy)
CATACLYSMIC variable stars
SYNCHROTRON radiation
ELECTROMAGNETIC waves
ELECTROMAGNETIC theory
Źródło :
Monthly Notices of the Royal Astronomical Society; 3/21/2016, Vol. 457 Issue 1, p887-901, 15p
Czasopismo naukowe
Tytuł :
An X-ray and Radio Study of the Varying Expansion Velocities in Tycho's Supernova Remnant.
Autorzy :
Williams BJ; CRESST/USRA and X-ray Astrophysics Laboratory, NASA GSFC, 8800 Greenbelt Road, Greenbelt, MD, Code 662.
Chomiuk L; Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA.
Hewitt JW; University of North Florida, Department of Physics, 1 UNF Drive, Jacksonville, FL 32224, USA.
Blondin JM; Department of Physics, North Carolina State University, Raleigh, NC 27695.
Borkowski KJ; Department of Physics, North Carolina State University, Raleigh, NC 27695.
Ghavamian P; Department of Physics, Astronomy, and Geosciences, Towson University, Towson, MD 21252.
Petre R; NASA GSFC, X-ray Astrophysics Laboratory, Greenbelt, MD 20771, USA.
Reynolds SP; Department of Physics, North Carolina State University, Raleigh, NC 27695.
Pokaż więcej
Źródło :
The astrophysical journal. Letters [Astrophys J Lett] 2016 Jun 01; Vol. 823 (2). Date of Electronic Publication: 2016 May 26.
Typ publikacji :
Journal Article
Czasopismo naukowe
Tytuł :
Identifying IGR J14091-6108 as a magnetic CV with a massive white dwarf using X-ray and optical observations.
Autorzy :
Tomsick, John A.
Rahoui, Farid
Krivonos, Roman
Clavel, MaÏca
Strader, Jay
Chomiuk, Laura
Pokaż więcej
Temat :
GAMMA-ray scattering
GALACTIC X-ray sources
X-ray astronomy
DWARF galaxies
Źródło :
Monthly Notices of the Royal Astronomical Society; 7/21/2016, Vol. 460 Issue 1, p513-523, 11p
Przedsiębiorstwo/ jednostka :
NATIONAL Optical Astronomy Observatories (U.S.)
Czasopismo naukowe
Tytuł :
Shock-powered radio emission from V5589 Sagittarii (Nova Sgr 2012 #1).
Autorzy :
Weston, Jennifer H. S.
Sokoloski, J. L.
Chomiuk, Laura
Linford, Justin D.
Nelson, Thomas
Mukai, Koji
Finzell, Tom
Mioduszewski, Amy
Rupen, Michael P.
Walter, Frederick M.
Pokaż więcej
Temat :
SOLAR radio emission
X-ray astronomy
ASTRONOMICAL observations
RADIO frequency
NOVAE (Astronomy)
Źródło :
Monthly Notices of the Royal Astronomical Society; 8/11/2016, Vol. 460 Issue 3, p2687-2692, 11p
Czasopismo naukowe

Ta witryna wykorzystuje pliki cookies do przechowywania informacji na Twoim komputerze. Pliki cookies stosujemy w celu świadczenia usług na najwyższym poziomie, w tym w sposób dostosowany do indywidualnych potrzeb. Korzystanie z witryny bez zmiany ustawień dotyczących cookies oznacza, że będą one zamieszczane w Twoim komputerze. W każdym momencie możesz dokonać zmiany ustawień dotyczących cookies