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1. Full Text Classical T Tauri stars: magnetic fields, coronae and star-disc interactions
by Johnstone, C. P and Jardine, M and Gregory, S. G and Donati, J.-F and Hussain, G
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2014, Volume 437, Issue 4, pp. 3202 - 3220
The magnetic fields of young stars set their coronal properties and control their spin evolution via the star-disc interaction and outflows. Using 14 magnetic... 
Variables | Activity-circumstellarmatter-stars | Pre-main sequence-stars | Stars | T Tauri | Coronae-stars | Herbig Ae/Be | Rotation-stars | Magnetic field-stars | MASS ACCRETION | NEUTRON-STARS | INCLINED DIPOLE | stars: variables: T Tauri | M DWARFS | stars: pre-main sequence | STELLAR CORONAE | stars: magnetic field | circumstellar matter | ASTRONOMY & ASTROPHYSICS | X-RAY-EMISSION | GLOBAL 3D SIMULATIONS | YOUNG STARS | MAGNETOSPHERIC ACCRETION | 3-DIMENSIONAL SIMULATIONS | stars: coronae | stars: activity | stars: rotation | Physics - Solar and Stellar Astrophysics
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2. Full Text S Coronae Australis
: a T Tauri twin
by Gahm, G. F and Petrov, P. P and Tambovsteva, L. V and Grinin, V. P and Stempels, H. C and Walter, F. M and Institutionen för fysik och astronomi and Fysiska sektionen and Teknisk-naturvetenskapliga vetenskapsområdet and Uppsala universitet
Astronomy and Astrophysics, ISSN 1432-0746, 2018, Volume 614
Context. The star S CrA is a tight visual binary consisting of two classical T Tauri stars. Both components are outstanding regarding their spectral... 
Fysik | Physical Sciences | Astronomi, astrofysik och kosmologi | Naturvetenskap | circumstellar matter | Natural Sciences | Herbig Ae/Be | stars: activity | stars: individual: S CrA | Astronomy, Astrophysics and Cosmology | stars: variables: T Tauri
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3. Full Text S Coronae Australis: A T Tauri twin
by Gahm, G.F and Petrov, P.P and Tambovsteva, L.V and Grinin, V.P and Stempels, H.C and Walter, F.M and Stockholms universitet and Naturvetenskapliga fakulteten and Institutionen för astronomi
Astronomy and Astrophysics, ISSN 0004-6361, 06/2018, Volume 614, p. A117
Context. The star S CrA is a tight visual binary consisting of two classical T Tauri stars. Both components are outstanding regarding their spectral... 
Stars: individual: S CrA | Circumstellar matter | Stars: variables: T Tauri, Herbig Ae/Be | Stars: activity | MAIN-SEQUENCE STARS | FORMING REGIONS | EMISSION-LINE | stars: variables: T Tauri, Herbig Ae/Be | LINE-DATA-BASE | MWC 480 | circumstellar matter | ASTRONOMY & ASTROPHYSICS | THERMAL STRUCTURE | MAGNETOSPHERIC ACCRETION | HERBIG AE/BE STARS | stars: activity | INTERMEDIATE-MASS STARS | stars: individual: S CrA | DISK-WIND | Stellar winds | Wind | Brightness | T Tauri stars | Spectral signatures | Surface chemistry | Luminosity | Accretion disks | Absorption | Spectrum analysis | Mathematical models | Numerical models | Photometry | Interferometry | Stellar spectra | Spectroscopy | Accretion | Parameters | Computer simulation | Extinction | Infrared signatures | Magnetospheres | Velocity | Emissions | European Southern Observatory | Photometric observations | Near infrared radiation | Photosphere | Brightness of stars | Binary stars | Stellar surfaces | Physics - Solar and Stellar Astrophysics | Fysik | Physical Sciences | Astronomi, astrofysik och kosmologi | Naturvetenskap | Natural Sciences | Herbig Ae/Be | Astronomy, Astrophysics and Cosmology | stars: variables: T Tauri
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4. R Coronae Borealis light curves
: 1996-2000
by Mattei, Janet A. (Janet Akyüz) and Menali, H. Gamze and Waagen, Elizabeth O and American Association of Variable Star Observers
2002, AAVSO monograph ; Supplement 2, ISBN 187817438X, Volume 4., x, 3 leaves
Variable stars | R Coronae Borealis stars
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5. Full Text Plasma astrophysics
: kinetic processes in solar and stellar coronae
by Benz, A. O and SpringerLink (Online service)
2002, 2nd ed., Astrophysics and space science library, ISBN 1402006950, Volume 279, 328
This textbook is intended as an introduction to the physics of solar and stellar coronae, emphasizing kinetic plasma processes. It is addressed to... 
Particle beams | Plasma astrophysics | Corona | Sun Corona | Stars | Plasma dynamics | Sun | Astrophysics and Astroparticles | Nuclear Physics, Heavy Ions, Hadrons | Planetology | Plasma Physics | Nuclear physics
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6. Full Text Chandra survey of nearby highly inclined disc galaxies - I. X-ray measurements of galactic coronae
by Li, Jiang-Tao and Wang, Q. Daniel
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2013, Volume 428, Issue 3, pp. 2085 - 2108
We present a systematical analysis of the Chandra observations of 53 nearby highly inclined (i 60°) disc galaxies to study the coronae around them. This sample... 
Galaxies | General-galaxies | Haloes-X-rays | galaxies: general | NORMAL ELLIPTIC GALAXIES | STAR-FORMING GALAXIES | X-rays: galaxies | TULLY-FISHER RELATION | DIFFUSE IONIZED-GAS | CLUSTER SCALING PROJECT | HOT INTERSTELLAR-MEDIUM | ASTRONOMY & ASTROPHYSICS | WIND CHARGE-EXCHANGE | XMM-NEWTON OBSERVATIONS | CENTRAL BLACK-HOLES | MULTIPHASE GASEOUS HALOS | galaxies: haloes
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7. R Coronae Borealis light curves
: 1991-1995
by Mattei, Janet A. (Janet Akyüz) and Waagen, Elizabeth O and Foster, E. Grant and American Association of Variable Star Observers
1996, AAVSO monograph, ISBN 9781878174178, Volume 4, Supplement 1, x, 3 leaves
Variable stars | Catalogs | R Coronae Borealis stars
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8. Orbit of [beta] Coronae Borealis
by Cannon, J.B
1914, Publications of the Dominion Observatory, Ottawa, Volume 1(14), [375]-405.
orbits | stars | astronomy
Book
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9. R Coronae Borealis light curves, 1843-1990
by Mattei, Janet A. (Janet Akyüz)
1991, AAVSO monograph., ISBN 9781878174031, Volume 4
Book
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10. Full Text R Coronae Borealis: radial velocity and other observations, 1950-2007
by Feast, MW and Griffin, RF and Herbig, GH and Whitelock, PA
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 01/2019, Volume 482, Issue 3, pp. 4174 - 4187
Radial-velocity observations made on more than a thousand nights are presented for the type star of the R Coronae Borealis (RCB) class. There are four... 
techniques: radial velocities | TELESCOPE | stars: variables: general | LIGHT | stars: carbon | stars: individual: R CrB | DECLINE | DUST | PHOTOMETRY | ASTRONOMY & ASTROPHYSICS | stars: peculiar | PERIOD | stars: mass-loss | STARS | Physics - Solar and Stellar Astrophysics
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11. Physics of solar and stellar coronae
: G.S. Vaiana Memorial Symposium : proceedings of a Conference of the International Astronomical Union, held in Palermo, Italy, 22-26 June, 1992
by Linsky, J. L and Serio, Salvatore
1993, Astrophysics and space science library, ISBN 9780792323464, Volume 183., xxv, 650
Corona | Congresses | Stars | Astronautics in astronomy
Book
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12. Full Text X-ray coronae in simulations of disc galaxy formation
by Crain, Robert A and McCarthy, Ian G and Frenk, Carlos S and Theuns, Tom and Schaye, Joop
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2010, Volume 407, Issue 3, pp. 1403 - 1422
The existence of X-ray luminous gaseous coronae around massive disc galaxies is a long-standing prediction of galaxy formation theory in the cold dark matter... 
galaxies: formation | X‐rays: galaxies | methods: numerical | galaxies: haloes | Galaxies: haloes | Galaxies: formation | X-rays: galaxies | Methods: numerical | COLD DARK-MATTER | ELLIPTIC GALAXIES | STAR-FORMATION | SMOOTHED PARTICLE HYDRODYNAMICS | COSMOLOGICAL SIMULATIONS | ROSAT PSPC OBSERVATIONS | ASTRONOMY & ASTROPHYSICS | LAMBDA-CDM HALOES | INTRACLUSTER ENTROPY | HOT GAS HALOS | HIGH-VELOCITY CLOUDS | Analysis | X-rays | Universities and colleges | Luminosity | X ray astronomy | Dark matter | Accretion disks | Stars & galaxies
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13. Full Text Accretion disk coronae of intermediate polar cataclysmic variables: 3D magnetohydrodynamic modelling and thermal X-ray emission
by Barbera, E and Orlando, S and Peres, G
Astronomy and Astrophysics, ISSN 0004-6361, 04/2017, Volume 600, p. A105
Context. Intermediate polar cataclysmic variables (IPCV) contain a magnetic, rotating white dwarf surrounded by a magnetically truncated accretion disk. To... 
Magnetohydrodynamics (MHD) | Novae, cataclysmic variables | Stars: coronae | X-rays: stars | Stars: flare | Accretion, accretion disks | INSTABILITY | accretion, accretion disks | MAGNETIZED STARS | ALGORITHM | INCLINED DIPOLE | novae, cataclysmic variables | stars: flare | PLASMA | V709 CASSIOPEIAE | ASTRONOMY & ASTROPHYSICS | YOUNG STARS | 3-DIMENSIONAL SIMULATIONS | CONDUCTION | stars: coronae | FLOWS | magnetohydrodynamics (MHD) | Coronas | Magnetohydrodynamics | X rays | Surface chemistry | Emission | Disks | Magnetic fields | Accretion disks
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14. Full Text Magnetohydrostatic modelling of stellar coronae
by MacTaggart, D and Gregory, S.G and Neukirch, T and Donati, J.-F
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2016, Volume 456, Issue 1, pp. 767 - 774
We introduce to the stellar physics community a method of modelling stellar coronae that can be considered to be an extension of the potential field. In this... 
MHD | Stars: coronae | Stars: magnetic field | Methods: analytical | stars: magnetic field | STAR | GLOBAL MAGNETIC TOPOLOGY | MAGNETOSTATIC ATMOSPHERES | ASTRONOMY & ASTROPHYSICS | methods: analytical | stars: coronae
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15. Full Text Evolving R Coronae Borealis stars with MESA
by Lauer, A and Chatzopoulos, E and Clayton, GC and Frank, J and Marcello, DC
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 09/2019, Volume 488, Issue 1, pp. 438 - 450
The R Coronae Borealis ( RCB) stars are rare hydrogen-deficient, carbon-rich supergiants. They undergo extreme, irregular declines in brightness of many... 
ROTATING MASSIVE STARS | PRESUPERNOVA EVOLUTION | stars: evolution | EXTREME HELIUM | binaries: close | ABUNDANCES | stars: abundances | RCB | ORIGIN | white dwarfs | HYDROGEN-DEFICIENT CARBON | ASTRONOMY & ASTROPHYSICS | WHITE-DWARF BINARIES | Physics - Solar and Stellar Astrophysics
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16. Full Text Galactic fountains and the rotation of disc-galaxy coronae
by Marinacci, Federico and Fraternali, Filippo and Nipoti, Carlo and Binney, James and Ciotti, Luca and Lonillo, Pasquale
Monthly Notices of the Royal Astronomical Society, ISSN 1365-2966, 08/2011, Volume 415, Issue 2, pp. 1534 - 1542
In galaxies like the Milky Way, cold (˜104 K) gas ejected from the disc by stellar activity (the so-called galactic-fountain gas) is expected to interact with... 
intergalactic medium | hydrodynamics | Galaxy: structure | turbulence | Galaxy: kinematics and dynamics | ISM: kinematics and dynamics | Hydrodynamics | Turbulence | Intergalactic medium | SPIRAL GALAXIES | THERMAL-INSTABILITY | X-RAY-ABSORPTION | EXTRAPLANAR GAS | MODELS | ASTRONOMY & ASTROPHYSICS | IONIZED-GAS | H I HALO | MILKY-WAY | HIGH-VELOCITY CLOUDS | KINEMATICS | Clouds | Fluid dynamics | Astronomy | Fluid mechanics | Corona | Astrophysics | Stars & galaxies | Physics - Astrophysics of Galaxies
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17. Full Text Cracking the Conundrum of F-supergiant Coronae
by Ayres, Thomas R
Astrophysical Journal, ISSN 0004-637X, 02/2018, Volume 854, Issue 2, p. 95
Chandra X-ray and HST far-ultraviolet (FUV) observations of three early-F supergiants have shed new light on a previous puzzle involving a prominent member of... 
X-rays: stars | stars: coronae | ultraviolet: stars | stars: late-type | stars: activity | LUMINOSITY | ASTRONOMY & ASTROPHYSICS | EMISSION | Physics - Solar and Stellar Astrophysics
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18. Magnetohydrostatic modelling of stellar coronae
by D MacTaggart and S G Gregory and T Neukirch and J-F Donati
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 02/2016, Volume 456, Issue 1, p. 767
  We introduce to the stellar physics community a method of modelling stellar coronae that can be considered to be an extension of the potential field. In this... 
Astrophysics | Corona | Magnetic fields | Star & galaxy formation | Gravity
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19. Full Text DENSITY DETERMINATIONS OF THE CORONAE OF COOL STARS USING A NEWLY ASSIGNED PAIR OF Fe XIV LINES IN THE SPECTRA OF alpha CANIS MINOR, alpha CENTAURI, AND THE SUN
by Beiersdorfer, P and Hell, N and Lepson, JK and Diaz, F and Ishikawa, Y and Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 12/2015, Volume 815, Issue 1, p. 3
We have identified a previously unassigned pair of lines between 169 and 170 angstrom in the coronae of cool stars. We attribute these lines to Fe XIV and show... 
CHANDRA-LETGS OBSERVATIONS | PROXIMA-CENTAURI | stars: individual (Procyon, Alpha Centauri) | atomic processes | X-RAY SPECTROSCOPY | Sun: X-rays, gamma-rays | HIPPARCOS | line: formation | ASTRONOMY & ASTROPHYSICS | EXTREME-ULTRAVIOLET | PROCYON | CAPELLA | stars: coronae | TRANSITIONS | EMISSION | DIAGNOSTICS | Gratings (spectra) | Cool stars | X-rays | Spectral lines | Diffraction gratings | Electron density | Density | Sun | line formation | Sun: X-rays | ATOMIC AND MOLECULAR PHYSICS | ASTRONOMY AND ASTROPHYSICS | gamma-rays | stars coronae | stars individual (Procyon, Alpha Centauri)
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