Stellar Coronae
Stellar coronae are hot ionized plasmas in the outer atmospheres of most
stars. X-ray spectra that are being obtained by the Chandra and
XMM-Newton observatories allow us to determine the thermal structure,
densities, and dynamics of stellar coronae. We have analyzed Chandra
spectra of late-type stars (stars with convective zones like the Sun) to infer
these properties and to determine the roles played by magnetic fields in
stellar coronae. The figure above shows Chandra spectrum of the dM1e
dwarf star AU Microscopii with the important emission lines marked. The top
panel is from the Medium Energy Grating (MEG) and the bottom panel is from the
High Energy Grating (HEG). Analysis of the line fluxes leads to the emission
measure distribution, electron densities, and a model for the coronal plasma of
the star.
Research Objectives:
- Analyze X-ray and EUV spectra of stars using the Chandra,
XMM-Newton, and EUVE satellites.
- Determine the physical properties and structure of the coronae of active
and quiescent late-type stars and binary systems.
- Search for X-ray emission from A and B-type stars.
- Study flare dynamics and energetics using high resolution X-ray and UV
spectra of coronal emission lines.
- Analyze the nonthermal radio emission from late-type stars.
Important Results and Discoveries:
- Described the relative emission from chromospheres and
coronae as a function of stellar effective temperature and age.
- Computed models of M dwarf stars that include coronae consistent
with the observed X-ray emission.
- Showed that the relative FIP effect in stars depends on spectral
type and activity.
- Surveyed the forbidden coronal emission lines in ultraviolet and
optical spectra and showed that their fluxes are consistent with
X-ray spectra.
- Obtained and analyzed multiwavelength (X-ray to optical) emission
of stars during quiescence and flaring.
- Reviewed the quiescent and flare X-ray emission, coronal mass
ejections, and stellar-planetary interactions in the book "Host Stars
and their effects on Exoplanet Atmospheres".
Papers published in refereed journals since 2000:
- Tilipman, D., Vieytes, M., Linsky, J.L., Buccino, A.P., and
France, K.: 2021, "Semiempirical Modeling of the Atmospheres of
the M Dwarf Exoplanet Hosts GJ 832 and GJ 581", Astrophysical
Journal, 909, 61
- Duvvuri, G.M., Sabastian Pineda, J., Berta-Thompson, Z.K.,
Linsky, J.L., et al.: 2021, "Reconstructing the extreme ultraviolet
emission of cool dwarfs using differential emission measure
polynomials", Astrophysical Journal, 913, 30D
- Linsky, J.L., Wood, B.E., Youngblood, A., Brown, A., et al.: 2020,
"The Relative Emission from Chromospheres and Coronae: Dependence
on Spectral Type and Age", Astrophysical Journal, 902, 3
- France, K., Duvvuri, G.M., Egan, H., Linsky, J.L.,et al.: 2020,
"The high-energy radiation environment around a 10 Gyr M dwarf:
Habitable at last?", Astronomical Journal, 160, 237
- Froning, C.S., Kowalski, A., France, K., Linsky, J.L., et al.:
2019, "The hot ultraviolet flare on the M dwarf GJ 674",
Astrophysical Journal, 871, 26F
- Loyd, R.OP., France, K., Youngblood, A., Schneider, C., Brown,
A., Hu, R., Linsky, J.L., et al.: 2016, " The MUSCLES Treasury
Survey. III. X-Ray to Infrared Spectra of 11 M and K Stars Hosting
Planets", Astrophysical Journal, 824, 102
- Wood, B.E. and Linsky, J.L.: 2010, "Resolving the Xi Boo binary
with Chandra, and revealing the spectral type dependence of the
corona 'FIP' effect", Astrophysical Journal, 717, 1279
- Wood, B.E. and Linsky, J.L.: 2006, "Coronal Emission Measures and
Abundances for Moderately Active K Dwarfs Observed by Chandra",
Astrophysical Journal, 643, 444
- Osten, R.A., Brown, A., Ayres, T.A., Drake, S.A., Franciosini, E.,
Pallavicini, R., Tagliaferri, G., Stewart, R.T., Skinner, S.L., and Linsky,
J.L.: 2004, "A multi-wavelength perspective of flares on HR 1099: Four years of
coordinated campaigns", Astrophysical Journal
Supplements, 153, 317
- Guedel, M., Audard, M., Reale, F., Skinner, S.L., and Linsky, J.L.: 2004,
"Flares from small to large: X-ray spectroscopy of Proxima Centauri with
XMM-Newton", Astronomy and Astrophysics, 416, 713
- Redfield, S., Ayres, T.R., Linsky, J.L., Ake, T.B., Dupree, A.K.,
Robinson, R.D., and Young, P.R.: 2003, "A Far Ultraviolet Spectroscopic
Explorer survey of coronal forbidden lines in late-type stars",
Astrophysical Journal, 585, 993
- Ayres, T.R., Brown, A., Harper, G.M., Osten, R.A., Linsky, J.L., Wood,
B.E., and Redfield, S.: 2003, "Space Telescope Imaging Spectrograph Survey of
far-ultraviolet coronal forbidden lines in late-type stars",
Astrophysical Journal, 583, 963
- Osten, R.A., Ayres, T.R., Brown, A., Linsky, J.L., and Krishnamurthi, A.:
2003, "Chandra, Extreme Ultraviolet Explorer, and Very Large Array observations
of the active binary system Sigma2 Coronae Borealis",
Astrophysical Journal, 582, 1073
- Daniel, K., Linsky, J.L., and Gagne, M.: 2002, "Chandra observations of
the Pleiades Open Cluster: X-ray emission from some late-B to early-A stars",
Astrophysical Journal, 578, 486
- Robinson, R.D., Linsky, J.L., Woodgate, B.E., and Timothy, J.G.: 2001,
"Far-ultraviolet observations of flares on the dM0e star AU Microscopii",
Astrophysical Journal, 554, 368
- Ayres, T.R., Brown, A., Osten, R.A., Huenemoerder, D.P., Drake, J.J.,
Brickhouse, N.S., and Linsky, J.L.: 2001, "Chandra, EUVE, Hubble, and VLA
multi-wavelength campaign on HR 1099: Instrumental capabilities, data
reduction, and initial results",
Astrophysical Journal, 549, 554
- Krishnamurthi, A., Reynolds, C.S., Linsky, J.L., Martin, E., and Gagne:
2001, "Observations of the core of the Pleiades with the Chandra X-ray
Observatory", Astronomical Journal, 121, 337
- Leto, G., Pagano, I., Linsky, J.L., Rodono, M., and Umana, G.: 2000,
"VLA observation of dMe stars",
Astronomy and Astrophysics, 359, 1035
- Osten, R.A., Brown, A., Ayres, T.R., Linsky, J.L., Drake, S.A., Gagne, M.,
and Stern, R.A.: 2000, "Radio, X-ray, and Extreme-Ultraviolet coronal
variability of the short-period RS Canum Venaticorum binary Sigma2 Coronae
Borealis",
Astrophysical Journal, 544, 953
Review Papers and conference papers since 2000:
- Linsky, J.: 2019, "Host Stars and their Effects on Exoplanet
Atmospheres", book published by Springer
- Forbich, J., Guedel, M., Linsky, J.L. et al.: 2011, "The
radio-X-ray relation in cool stars: Are we headed toward a
divorce?", in The 16th Cambridge Workshop on Cool Stars,
Stellar Systems and the Sun, ed. C.M. Johns-Krull, M.K. Browning,
and A.A. West, ASP Conf. Series, 448, 455
- Lillie, C., Cash, W., Arav, N., Shull, J.M., and Linsky, J.L.:
2007, "High resolution soft X-ray spectroscopy for Constellation X",
SPIE 6686, 668612
- Linsky, J.L., Gagne', M., Mytyk, A., McCaughren, M., and
Andersen, M.: 2008, "The Eagle Nebula: Pillars of Creation, EGGs,
and PMS Stars in NGC 6611", in 14th
Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun, ed.
G.T. van Belle, Astronomical Society of the Pacific Conference
Series, 384, 59
- Linsky, J.L., Gagne', M., Mytyk, A., McCaughren, M., and
Andersen, M.: 2007, "Chandra Observations of the Eagle Nebula. I.,
Embedded Young Stellar Objects near the Pillars of Creation",
Astrophysical Journal, 654, 347
- Linsky, J.L.: 2006, "Stellar Magnetic Fields and Signatures of Heating",
invited paper presented at session D2.2/E3.2 of the COSPAR meeting in Beijing,
China, July 17, 2006,
powerpoint presentation
- Linsky, J.L.: 2004, "Summary of Cool Stars, Stellar Systems, and the Sun",
powerpoint presentation
- Linsky, J.L.: 2003, "X-ray coronae of stars: Recent results from Chandra",
Advances in Space Research, 32, No. 6, 917
- Linsky, J.L.: 2003, "Why high spectral resolution is needed for the
Constellation-X mission",
Presentation given at the Constellation-X Spectroscopy
Workshop 2003, Columbia University
- Linsky, J.L., Ayres, T.R., Brown, A., and Osten, R.A.: 2002, "Comparison
of the spectrum of a sunspot-like star with a sunspot",
Astronomische Nachrichten, 323, 321
- Linsky, J.L.: 2002, "Historical perspective -- Lessons learned and lessons
to be learned", in Stellar Coronae in the Chandra and XMM Era, ed. F. Favata
and J. Drake, ASP Conf. Series, 277, 3
- Linsky, J.L.: 2002, "Crazy coronal abundances",
in X-rays at Sharp Focus, ASP Conf. Series, 262, 45
- Linsky, J.L., Ayres, T.R., Brown, A., Osten, R., Skinner, S., and Gagne,
M.: 2001, "Stellar coronae: new insights into fundamental questions", in New
Century of X-ray Astronomy,
ASP Conf. Series, 251, 22
- Linsky, J.L., Skinner, S., Osten, R., Gagne, M.: 2001, "Chandra spectra of
three very active stars: AB Dor, 44i Boo, and Sigma2 CrB",
in X-RAY Astronomy 2000, ed. R. Giaconni, L. Stella, and S. Serio,
ASP Conf. Series, 234, 65
- Linsky, J.L., Skinner, S., Osten, R., Gagne, M.: 2001, "Chandra spectra of
four very active stars: AB Dor, 44i Boo, and Sigma2 CrB and AU Mic",
in Magnetic Fields Across the Hertzsprung-Russell Diagram, ed. G. Mathys, S.K.
Solanki, and D.T. Wickramasinghe,
ASP Conf. Series, 248, 255
- Linsky, J.L.: 2000, "Stellar flares: How common? How important?", in
Cosmic Explosions, ed. S.S. Holt and W.W. Zhang
(Melville NY: Am. Institute of Physics), p. 389
- Linsky, J.L., Krishnamurthi, A., Gagne, M., and Guedel, M.: 2000, "Are the
shapes of coronal emission measure distributions controlled by rotation and
convection zone parameters?", in Stellar Clusters and Associations, ed. R.
Pallavicini, G. Micela, and S. Sciortino (San Francisco: Astron. Soc. Pacific),
p. 467
- Linsky, J.L.: "Comparing solar and stellar activity: new results from HST,
Chandra, and XMM", invited talk at the American Astronomical Society Solar
Physics Division meeting, State Line, NV, June 20, 2000
- Linsky, J.L.: 2000, "Microarcsecond X-ray imaging of stars", invited talk
at the
MAXIM Pathfinder Mission Definition Team meeting,
Goddard Space Flight Center, Greenbelt MD, Sept 18, 2000
- Linsky, J.L.: 2000, "What have we learned? Where are we going? And some
lessons from the past", in
Stellar Clusters and Associations, ed. R.
Pallavicini, G. Micela, and S. Sciortino (San Francisco: Astron. Soc.
Pacific), p. 563
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