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Items where Person is "Edwards-S"

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Number of items: 14.

2015

Pascucci, I. and Edwards, S. and Heyer, M. et al. (2015) Narrow Na and K Absorption Lines Toward T Tauri Stars: Tracing the Atomic Envelope of Molecular Clouds. Astrophysical Journal, 814 (1). Art. No. 14. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20160105-141144006

Rigliaco, Elisabetta and Pascucci, I. and Duchene, G. et al. (2015) Probing Stellar Accretion with Mid-infrared Hydrogen Lines. Astrophysical Journal, 801 (1). Art. No. 31. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20150403-141146223

2014

McJunkin, Matthew and France, Kevin and Schneider, P. C. et al. (2014) Direct Measurement of Interstellar Extinction toward Young Stars Using Atomic Hydrogen Lyα Absorption. Astrophysical Journal, 780 (2). Art. No. 150. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20140218-153756605

2013

Edwards, Suzan and Kwan, John and Fischer, William et al. (2013) Interpreting Near Infrared Hydrogen Line Ratios in T Tauri Stars. Astrophysical Journal, 778 (2). Art. No. 148. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20140106-141752262

Ardila, David R. and Herczeg, Gregory J. and Gregory, Scott G. et al. (2013) Hot Gas Lines in T Tauri Stars. Astrophysical Journal Supplement Series, 207 (1). Art. No. 1. ISSN 0067-0049. https://resolver.caltech.edu/CaltechAUTHORS:20130904-133609652

Ingleby, Laura and Calvet, Nuria and Herczeg, Gregory et al. (2013) Accretion Rates for T Tauri Stars Using Nearly Simultaneous Ultraviolet and Optical Spectra. Astrophysical Journal, 767 (2). Art. No. 112. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20130521-140050828

2011

Ingleby, Laura and Calvet, Nuria and Bergin, Edwin et al. (2011) Near-ultraviolet Excess in Slowly Accreting T Tauri Stars: Limits Imposed by Chromospheric Emission. Astrophysical Journal, 743 (2). Art. No. 105. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20120201-112949727

Fischer, William and Edwards, Suzan and Hillenbrand, Lynne et al. (2011) Characterizing the IYJ Excess Continuum Emission in T Tauri Stars. Astrophysical Journal, 730 (2). Art. No. 73. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20110414-085412533

2010

Sharon, Chelsea and Hillenbrand, Lynne and Fischer, William et al. (2010) F, G, K, M Spectral Standards in the Y Band (0.95-1.11 μm). Astronomical Journal, 139 (2). pp. 646-667. ISSN 0004-6256. https://resolver.caltech.edu/CaltechAUTHORS:20100208-114500344

2008

Fischer, William and Kwan, John and Edwards, Suzan et al. (2008) Redshifted absorption at He I λ10830 as a probe of the accretion geometry of T Tauri stars. Astrophysical Journal, 687 (2). pp. 1117-1144. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20090924-202018155

2006

Edwards, Suzan and Fischer, William and Hillenbrand, Lynne et al. (2006) Probing T Tauri accretion and outflow with 1 micron spectroscopy. Astrophysical Journal, 646 (1). pp. 319-341. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:EDWapj06

2003

Edwards, Suzan and Fischer, William and Kwan, John et al. (2003) He I λ10830 as a probe of winds in accreting young stars. Astrophysical Journal Letters, 599 (1). L41-L44. ISSN 2041-8205. https://resolver.caltech.edu/CaltechAUTHORS:EDWapjl03

Edwards, Shaune and Li, Caroline M. and Levy, Daniel L. et al. (2003) Saccharomyces cerevisiae DNA Polymerase ε and Polymerase σ Interact Physically and Functionally, Suggesting a Role for Polymerase ε in Sister Chromatid Cohesion. Molecular and Cellular Biology, 23 (8). pp. 2733-2748. ISSN 0270-7306. PMCID PMC152548. https://resolver.caltech.edu/CaltechAUTHORS:20111011-085516908

2000

Dua, Rajiv and Edwards, Shaune and Levy, Daniel L. et al. (2000) Subunit interactions within the Saccharomyces cerevisiae DNA polymerase ε (pol ε) complex - Demonstration of a dimeric pol ε. Journal of Biological Chemistry, 275 (37). pp. 28816-28825. ISSN 0021-9258. https://resolver.caltech.edu/CaltechAUTHORS:DUAjbc00

This list was generated on Sun Aug 9 05:17:01 2020 PDT.