'Line profiles' diaporamas de présentation

Nicolas GREVESSE*

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A database for water transitions from experiment and theory

A database for water transitions from experiment and theory. Jonathan Tennyson HITRAN meeting Department of Physics and Astronomy Harvard University College London June 2006.

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Accretion Processes in Star Formation Lee Hartmann Cambridge Astrophysics Series, 32

(continued). Accretion Processes in Star Formation Lee Hartmann Cambridge Astrophysics Series, 32 Cambridge University Press (also from Nuria Calvet talks (2004). Energetic Problem in TTS. CTTS, L bol > L * ( > 10% on average). An additional source of energy is required.

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SPOTS AND GRANULATION as a Function of Mass and Age

SPOTS AND GRANULATION as a Function of Mass and Age. Mark Giampapa National Solar Observatory Tucson, Arizona USA. Granulation. First and most apparent non-uniformity observed in the Quiet Sun Bright cells of irregular polygonal shape separated by dark lanes

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The CoRoT ground-based complementary archive

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What can we learn on the BLR from the smallest AGN?

What can we learn on the BLR from the smallest AGN?. Or, how do the BLR properties change with luminosity, and what is it telling us? Specifically The BLR radius vs. luminosity The BL profiles vs. luminosity Objects without a BLR. The AGN Paradigm. Is it luminosity dependent?.

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Stellar Spectroscopy during Exoplanet Transits Revealing structures across stellar surfaces

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Analysis of Doppler-Broadened X-ray Emission Line Profiles from Hot Stars

Analysis of Doppler-Broadened X-ray Emission Line Profiles from Hot Stars. David Cohen - Swarthmore College with Roban Kramer - Swarthmore College Stanley Owocki - Bartol Research Institute. Outline. 0. The astrophysical context I. Introduction: What line profiles can tell us

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Sunspot Studies in Oslo with CDS,SUMER,MDI and TRACE A final report (maybe).

Sunspot Studies in Oslo with CDS,SUMER,MDI and TRACE A final report (maybe). Olav Kjeldseth-Moe, Per Maltby , Terje Fredvik and Nils Brynildsen Institute of Theoretical Astrophysics University of Oslo. Program History. Sunspot studies with SOHO instruments from 06/1996.

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Stellar Spectroscopy during Exoplanet Transits

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NIRI Observations of Type Ia Supernovae

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PhD Students of Jeffrey Linsky

PhD Students of Jeffrey Linsky. Richard Shine (1973) George Mount (1975) Thomas Ayres (1975) Douglas Brown (1975) Gibor Basri (1979) Patricia Bornmann (1985). James Neff (1987) Steven Saar (1987) Stephen Skinner (1992) Brian Wood (1996) Seth Redfield (2003) Gregory Herczeg (2005).

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PhD Students of Jeffrey Linsky

PhD Students of Jeffrey Linsky. Richard Shine (1973) George Mount (1975) Thomas Ayres (1975) Douglas Brown (1975) Gibor Basri (1979) Patricia Bornmann (1985). James Neff (1987) Steven Saar (1987) Stephen Skinner (1992) Brian Wood (1996) Seth Redfield (2003) Gregory Herczeg (2005).

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Infall rates from observations

Infall rates from observations. Joseph Mottram. Why is infall relevant?. Infall must happen for star formation to proceed The rate of infall on envelope scales is important for the t imescale for envelope depletion

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ATOMDB Work Week @ CfA 2012 August 6-10

Plasma models of calibration sources at high resolution Andy Pollock XMM-Newton RGS Calibration Scientist IACHEC High-Resolution Working Group. ATOMDB Work Week @ CfA 2012 August 6-10. HETG spectra and old APEC model of Capella. MEG HEG. HETG spectra and old APEC model of Capella. MEG HEG.

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EUV Doppler shifts as a Signature of Transient Heating in the Solar Corona

EUV Doppler shifts as a Signature of Transient Heating in the Solar Corona. Youra Taroyan & Keiran Burrows BUKS Meeting 5 July 2012. Pre-Hinode EUV Doppler shift measurements. Peter & Judge (1999) Teriaca et al. (1999). Hinode / EIS. Hara et al. 2008, etc.

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LINE PROFILES & WAVELENGTHS ACROSS STELLAR SURFACES

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3-D study of the expansion of the nebula of the symbiotic Mira He2-147

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Synthetic Analysis of a Two-ribbon Microflare

Synthetic Analysis of a Two-ribbon Microflare. C. Fang, R. L. Jiang, P. F. Chen, Y. H. Tang. Department of Astronomy, Nanjing University, Nanjing, China ( fangc@nju.edu.cn ). Abstract.

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Congresso del Dipartimento di Fisica Highlights in Physics 2005

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