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)

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 (A+A 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)

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) λ3144 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)

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. α Centauri A (G2V) and α Centauri B (K1V) (ApJ 210, 199, 1976)

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)

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 β Draconis, Geminorum, and α Orionis (ApJ 251, 162, 1981)

• Formation of chromospheric resonance line profiles in supergiants (ApJ 242, 1133, 1980)

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)

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 (A+A 176, 267, 1987)

• …IV. The spatially resolved chromosphere of AR Lacertae (A+A 186, 241, 1987)

• …XI. Ultraviolet spectral images of AR Lacertae in September 1985 (A+A 215, 79, 1989)

• Spectral images and multicomponent models of the chromospheres of AR Lacertae (PASP 100, 407, 1988)

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)

Stephen Skinner (1992): Radio Emission from Pre-main-sequence Stars

• New radio detections of early-type pre-main-sequence stars (ApJ 357, L39, 1990)

• BD+24°676 – an intermediate-mass, pre-main-sequence star (PASP 102, 754, 1990)

• Nonthermal radio emission from the X-ray bright K5 IV star 1E1751+7046 (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)

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)

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 Capella’s corona: GHRS spectra of the Fe XXI λ1354 and He II λ1640 lines from each of the Capella stars (ApJ 492, 767, 1998)

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)

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)

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)

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 Lyα 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)