Herschel SPIRE and PACS observations of the red supergiant VY CMa: analysis of the molecular line spectra
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Belgium | Canada. | Spain. | UK. | E. Observatory | M. Barlow | K. Leuven | J. Blommaert | J. Cernicharo | B. Swinyard | L. Decin | M. Groenewegen | M. Matsuura | R. Laboratory | J. Yates | E. Polehampton | R. Wesson | P. Royer | G. V. Steene | INTA-CSIC | P. J. U. C. London | Chile University of Lethbridge | Royal Observatory of Belgium | G. V. D. Steene
[1] N. Scoville,et al. OH-IR stars. I. Physical properties of circumstellar envelopes , 1976 .
[2] K. Nordsieck,et al. The Size distribution of interstellar grains , 1977 .
[3] On the origin of the grain-size spectrum of interstellar dust , 1980 .
[4] H. M. Lee,et al. Optical properties of interstellar graphite and silicate grains , 1984 .
[5] A. Sauval,et al. A set of partition functions and equilibrium constants for 300 diatomic molecules of astrophysical interest , 1984 .
[6] P. Goldsmith,et al. HCN emission from OH infrared sources , 1985, Nature.
[7] G. B. Scharmer,et al. A new approach to multi-level non-LTE radiative transfer problems , 1985 .
[8] H. Müller,et al. Submillimeter, millimeter, and microwave spectral line catalog. , 1985, Applied optics.
[9] G. Thomas. Infrared Astronomical Satellite (IRAS). , 1986 .
[10] M. Schenewerk,et al. Detection of hydrogen cyanide emission from the peculiar oxygen–rich evolved star IRC + 10420 , 1986, Nature.
[11] C. Beichman,et al. Infrared Astronomical Satellite (IRAS) catalogs and atlases , 1988 .
[12] P. J. Huggins,et al. The photodissociation of CO in circumstellar envelopes , 1988 .
[13] W. D. Watson,et al. Interacting masers and the extreme brightness of astrophysical water masers , 1989 .
[14] M. Rowan-Robinson,et al. Radiative transfer in axisymmetric dust clouds , 1990, Monthly Notices of the Royal Astronomical Society.
[15] S. Deguchi,et al. H2O emission from evolved stars at the far-infrared and submillimeter wavelengths , 1990 .
[16] G. Melnick,et al. Excitation of millimeter and submillimeter water masers , 1991 .
[17] Herbert M. Pickett,et al. The fitting and prediction of vibration-rotation spectra with spin interactions , 1991 .
[18] A. D. McLean,et al. Improved collisional excitation rates for interstellar water. , 1993, The Astrophysical journal. Supplement series.
[19] S. Langhoff,et al. A theoretical study of the electric dipole moment function of SiO , 1993 .
[20] C. Townes,et al. Characteristics of dust shells around 13 late-type stars. , 1994 .
[21] K. Menten,et al. Discovery of Strong Vibrationally Excited Water Masers at 658 GHz toward Evolved Stars , 1995 .
[22] A. Tielens,et al. Organic molecules in oxygen-rich circumstellar envelopes: methanol and hydrocarbons , 1995 .
[23] M. Kaufman,et al. Far-Infrared Water Emissions from Magnetohydrodynamic Shock Waves , 1996 .
[24] J. Yates,et al. NON-LOCAL RADIATIVE TRANSFER FOR MOLECULES : MODELLING POPULATION INVERSIONS IN WATER MASERS , 1997 .
[25] J. Yates,et al. High-frequency SiO masers in long-period variable stars , 1997 .
[26] D. Neufeld,et al. Models for Dense Molecular Cloud Cores , 1997, astro-ph/9707171.
[27] J. Yates,et al. MERLIN observations of water maser proper motions in VY Canis Majoris , 1998 .
[28] Observatoire de la Cote d'Azur,et al. The last gasps of VY Canis Majoris: Aperture synthesis and adaptive optics imagery , 1998 .
[29] P. Goldsmith,et al. Population Diagram Analysis of Molecular Line Emission , 1999 .
[30] J. Rawlings,et al. Modelling line profiles in infalling cores , 2001 .
[31] T. Onaka,et al. The time variation in infrared water-vapour bands in Mira variables , 2002, astro-ph/0201084.
[32] K. Leuven,et al. Mass loss and rotational CO emission from Asymptotic Giant Branch stars , 2003, astro-ph/0305207.
[33] S. Price,et al. A Uniform Database of 2.4-45.4 Micron Spectra from the Infrared Space Observatory Short Wavelength Spectrometer , 2003 .
[34] H. Bischof,et al. The Photodetector Array Camera and Spectrometer (PACS) on the Herschel Space Observatory , 2010, 1005.1487.
[35] C. Kramer,et al. The Herschel-Heterodyne Instrument for the Far-Infrared (HIFI) , 2005, Infrared and Millimeter Waves, Conference Digest of the 2004 Joint 29th International Conference on 2004 and 12th International Conference on Terahertz Electronics, 2004..
[36] P. J. Storey,et al. The dusty MOCASSIN: fully self-consistent 3D photoionization and dust radiative transfer models , 2005, astro-ph/0507050.
[37] Holger S. P. Müller,et al. The Cologne Database for Molecular Spectroscopy, CDMS: a useful tool for astronomers and spectroscopists , 2005 .
[38] C. Balança,et al. Rotational excitation of SiO by collisions with helium , 2006 .
[39] A. de Koter,et al. Probing the mass-loss history of AGB and red supergiant stars from CO rotational line profiles - I. Theoretical model – Mass-loss history unravelled in VY CMa , 2006, astro-ph/0606299.
[40] S. Kwok,et al. The Molecular Envelope around the Red Supergiant VY CMa , 2006, astro-ph/0611547.
[41] K. Menten,et al. Submillimeter vibrationally excited water emission from the peculiar red supergiant VY Canis Majoris , 2006, astro-ph/0606057.
[42] J. Tennyson,et al. A high-accuracy computed water line list , 2006, astro-ph/0601236.
[43] N. Woolf,et al. Chemical complexity in the winds of the oxygen-rich supergiant star VY Canis Majoris , 2007, Nature.
[44] Terry J. Jones,et al. The Three-Dimensional Morphology of VY Canis Majoris. I. The Kinematics of the Ejecta* , 2007 .
[45] David A. Naylor,et al. Apodizing functions for Fourier transform spectroscopy , 2007 .
[46] S. Sakai,et al. Distance to VY Canis Majoris with VERA , 2008, 0808.0641.
[47] E. Josselin,et al. Collisional excitation of water in warm astrophysical media - I. Rate coefficients for rovibrationally excited states , 2008 .
[48] K. Menten,et al. A multi-transition submillimeter water maser study of evolved stars. Detection of a new line near 475 GHz , 2007, 0710.5225.
[49] N. Woolf,et al. CIRCUMSTELLAR 12C/13C ISOTOPE RATIOS FROM MILLIMETER OBSERVATIONS OF CN AND CO: MIXING IN CARBON- AND OXYGEN-RICH STARS , 2008 .
[50] N. Woolf,et al. CARBON CHEMISTRY IN THE ENVELOPE OF VY CANIS MAJORIS: IMPLICATIONS FOR OXYGEN-RICH EVOLVED STARS , 2009 .
[51] G. Mcintosh,et al. Evidence for Stable v = 0, j = 1 → 0 SiO Maser Emission from VY Canis Majoris , 2009 .
[52] N. Woolf,et al. THE ARIZONA RADIO OBSERVATORY 1 mm SPECTRAL SURVEY OF IRC +10216 AND VY CANIS MAJORIS (215–285 GHz) , 2010 .
[53] K. Menten,et al. Polarisation observations of VY Canis Majoris H2O 532–441 620.701 GHz maser emission with HIFI , 2010, 1007.0905.
[54] K. Menten,et al. Probing the mass-loss history of AGB and red supergiant stars from CO rotational line profiles. II. CO line survey of evolved stars: derivation of mass-loss rate formulae , 2010, 1008.1083.
[55] M. Barlow,et al. Chemical and radiative transfer modelling of the ISO-LWS Fabry-Perot spectra of Orion-KL water lines , 2010, 1002.2111.
[56] D. Witherick,et al. Herschel -SPIRE FTS spectroscopy of the carbon-rich objects AFGL 2688, AFGL 618, and NGC 7027 , 2010, 1005.3279.
[57] S. Ott,et al. Herschel Space Observatory - An ESA facility for far-infrared and submillimetre astronomy , 2010, 1005.5331.
[58] R. C. Forrey,et al. ROTATIONAL QUENCHING OF CO DUE TO H2 COLLISIONS , 2010, 1004.3923.
[59] K. Menten,et al. Herschel/HIFI deepens the circumstellar NH3 enigma , 2010, 1007.1413.
[60] K. Menten,et al. The ISO Long Wavelength Spectrometer line spectrum of VY Canis Majoris and other oxygen-rich evolved stars , 2009, 0912.1626.
[61] Robert Mann,et al. Astronomical Data Analysis Software and Systems XXI , 2012 .
[62] S. J. Liu,et al. Herschel : the first science highlights Special feature L etter to the E ditor The Herschel-SPIRE instrument and its in-flight performance , 2010 .
[63] Kevin Xu,et al. The data processing pipelines for the Herschel/SPIRE imaging Fourier transform spectrometer , 2010, Astronomical Telescopes + Instrumentation.
[64] Michael J. Ireland,et al. Dynamical opacity-sampling models of Mira variables – II. Time-dependent atmospheric structure and observable properties of four M-type model series , 2011, 1107.3619.
[65] O. Krause,et al. MESS (Mass-loss of Evolved StarS), a Herschel key program , 2010, 1012.2701.
[66] K. Menten,et al. Herschel/HIFI observations of O-rich AGB stars : molecular inventory ⋆ , 2011, 1111.5156.
[67] K. Menten,et al. Pure rotational spectra of TiO and TiO2 in VY Canis Majoris , 2013, 1301.4344.