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PhD Students of Jeffrey Linsky

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... (1973): Physical Properties of Solar Plages. Physical properties of solar ... Brian Wood (1996): The Physical Properties and Dynamics of Stellar Transition ... – PowerPoint PPT presentation

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Title: PhD Students of Jeffrey Linsky


1
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)

2
Richard Shine (1973) Physical Properties of
Solar Plages
  • Physical properties of solar chromospheric
    plages. I. Line profiles of the Ca II H, K, and
    IR triplet lines (SoPh 25, 357, 1972)
  • Line profiles and turbulence generated by
    acoustic waves in the solar chromosphere. II.
    Contours of the CaII K and MgII k lines (AA 29,
    7, 1973)
  • A facular model based on the wings of the CaII
    lines (SoPh 37, 145, 1974)
  • Physical properties of solar chromospheric
    plages. II. Chromospheric plage models (SoPh 39,
    49, 1974)

3
George Mount (1975) Models of the Upper
Photospheres of the Sun and Arcturus based on
Molecular Spectra
  • One- and multi-component models of the upper
    photosphere based on molecular spectra. I., The
    violet system of CN (0,0) (SoPh 32,13, 1973)
  • II. CN (1,1) of the CN violet system (SoPh 35,
    259, 1974)
  • III. CH (0,0) ?3144 of the CH C-X system (SoPh
    36, 287, 1974)
  • IV. Non-LTE treatment of the CN violet system
    (SoPh 41, 17, 1975)
  • A non-LTE analysis of the CN 3883Å band head in
    the upper photosphere of Arcturus (ApJ 200, 383,
    1975)
  • A new solar carbon abundance based on non-LTE CN
    molecular spectra (ApJ 202, l51, 1975)

4
Thomas Ayres (1975) The Lower Chromospheres and
Upper Photospheres of Late-type Stars
  • Stellar model chromospheres. I. On the
    temperature minima of F, G, and K stars (ApJ 180,
    473, 1973)
  • II. Procyon (F5 IV-V) (ApJ 192, 93, 1974)
  • III. Arcturus (K2 III) (ApJ 200, 660, 1975)
  • IV. The formation of the H? feature in the Sun
    (G2 V) and Arcturus (K2 III) (ApJ 201, 212, 1975)
  • V. a Centauri A (G2V) and a Centauri B (K1V)
    (ApJ 210, 199, 1976)

5
Thomas Ayres (continued)
  • A possible width-luminosity correlation of the Ca
    K1 and Mg k1 features (ApJ 195, L121, 1975)
  • Resonance line transfer with partial
    redistribution. III. MgII resonance lines in
    solar-type stars (ApJ 197, 143, 1975)
  • Semiempirical upper photosphere models the Sun
    (G2V) and Procyon (F5 IV-V) (ApJ 201, 799, 1975)
  • The Mg II h and k lines. II. Comparison with
    synthesized profiles and Ca II K (ApJ 205, 874,
    1976)

6
Gibor Basri (1979) Supergiant Chromospheres
  • Outer atmospheres of cool stars. II. Mg II flux
    profiles and chromospheric radiative loss rates
    (ApJ 234, 1023, 1979)
  • VII. High resolution, absolute flux profiles of
    Mg II h and k lines in stars of spectral type F8
    to M5 (ApJS 44, 383, 1980)
  • VIII. IUE observations and chromospheric models
    for the supergiant stars ß Draconis, ? Geminorum,
    and a Orionis (ApJ 251, 162, 1981)
  • Formation of chromospheric resonance line
    profiles in supergiants (ApJ 242, 1133, 1980)

7
Patricia Bornmann (1985) Properties of Solar
Flare Plasmas Derived from Soft X-ray Line
Emission
  • A new method for determining temperature and
    emission measure during solar flares from light
    curves of soft X-ray line fluxes (ApJ 293, 595,
    1985)
  • Further analysis of temperature and emission
    measure during the decay phase of solar flares
    derived from soft X-ray light curves (SoPh 102,
    111, 1985)
  • Turbulence as a contributor to intermediate
    energy storage during solar flares (ApJ 313, 449,
    1987)

8
James Neff (1987) Spectral Images and
Multi-component Models of the Chromospheres of AR
Lacertae
  • Rotational modulation and flares on RS CVn and BY
    Dra stars. III. IUE observations of V711 Tau (HR
    1099), II Peg, and AR Lac (AA 176, 267, 1987)
  • IV. The spatially resolved chromosphere of AR
    Lacertae (AA 186, 241, 1987)
  • XI. Ultraviolet spectral images of AR Lacertae
    in September 1985 (AA 215, 79, 1989)
  • Spectral images and multicomponent models of the
    chromospheres of AR Lacertae (PASP 100, 407, 1988)

9
Steven Saar (1987) Observations and Analysis of
the Photospheric Magnetic Fields on the Dwarf G,
K, and M Stars
  • The photospheric magnetic field of the dM3.5e
    flare star AD Leonis (ApJ 299, L47, 1985)
  • The magnetic field of the BY Draconis star EQ
    Virginis (ApJ 302, 777, 1986)
  • Improved methods for the measurement and analysis
    of stellar magnetic fields (ApJ 324, 441, 1988)

10
Stephen Skinner (1992) Radio Emission from
Pre-main-sequence Stars
  • New radio detections of early-type
    pre-main-sequence stars (ApJ 357, L39, 1990)
  • BD24676 an intermediate-mass,
    pre-main-sequence star (PASP 102, 754, 1990)
  • Nonthermal radio emission from the X-ray bright
    K5 IV star 1E17517046 (ApJ 368, 272, 1991)
  • A search for evidence of cold dust around naked T
    Tauri stars (AJ 102, 1742, 1991)
  • Circularly polarized radio emission from the T
    Tauri star Hubble 4 (ApJ 408, 660, 1993)
  • A high-sensitivity survey of radio continuum
    emission from Herbig Ae/Be stars (ApJS 87, 217,
    1993)

11
Brian Wood (1996) The Physical Properties and
Dynamics of Stellar Transition Regions based on
High Resolution Ultraviolet Spectra
  • High-velocity plasma in the transition region of
    AU Microscopii Evidence for magnetic
    reconnection and saturated heating during
    quiescent and flaring conditions (ApJ 430, 342,
    1994)
  • The transition regions of Capella (ApJ 442, 381,
    1995)
  • A reanalysis of the SWP-HI IUE observations of
    Capella (ApJ 443, 329, 1995)

12
Brian Wood (continued)
  • Goddard High-Resolution Spectrograph observations
    of Procyon and HR 1099 (ApJ 458, 761, 1996)
  • Evaluating possible heating mechanisms using the
    transition region line profiles of late-type
    stars (ApJ 478, 745, 1997)
  • Dissecting Capellas corona GHRS spectra of the
    Fe XXI ?1354 and He II ?1640 lines from each of
    the Capella stars (ApJ 492, 767, 1998)

13
Seth Redfield (2003) The Three-dimensional
Physical Structure of the Local Interstellar
Medium
  • The three-dimensional structure of the warm LISM.
    I. Methodology (ApJ 528, 756, 2000)
  • II. The Colorado Model of the Local Interstellar
    Cloud (ApJ 534, 825, 2000)
  • Microstructure of the Local Interstellar Cloud
    and the identification of the Hyades Cloud (ApJ
    551, 413, 2001)
  • Elemental abundances and ionization states within
    the LIC from HST and FUSE observations of the
    Capella line of sight (ApJ 581, 1168, 2002)

14
Seth Redfield (continued)
  • The structure of the Local Interstellar Medium. I
    High-resolution observations of Fe II, Mg II, and
    Ca II toward stars within 100 parsecs (ApJS 139,
    439, 2002)
  • II. Observations of D I, C II, N I, O I, Al II,
    and Si II toward stars within 100 parsecs (ApJ
    602, 776, 2004)
  • III. Temperature and turbulence (ApJ 613, 1004,
    2004)

15
Gregory Herczeg (2005) Molecular Hydrogen
Fluorescence and Accretion in FUV Spectra of T
Tauri Stars
  • The far-ultraviolet spectrum of TW Hydrae. I.
    Observations of H2 fluorescence (ApJ 572, 310,
    2002)
  • II. Models of H2 fluorescence in a disk (ApJ
    607, 369, 2004)
  • Mapping the circumstellar environment of T Tauri
    with fluorescent H2 emission (AJ 126, 3076, 2003)
  • The loopy ultraviolet line profiles of RU Lupi
    Accretion, outflows, and fluorescence (AJ 129,
    2777, 2005)

16
Gregory Herczeg (continued)
  • The origin of fluorescent H2 emission in an
    HST/STIS survey of T Tauri stars (to be submitted
    to ApJ)
  • Reconstructing the hidden Lya emission from
    classical T Tauri stars (to be submitted to ApJ)
  • Probing accretion, winds, and H2 fluorescence in
    the FUSE spectrum of the CTTS TW Hya (to be
    written)
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