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On the Nature of Organic Dust in Novae

The Astrophysical journal, 2021-08, Vol.917 (2), p.103

2021

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The Three-Dimensional Morphology of VY Canis Majoris. I. The Kinematics of the Ejecta

The Astronomical journal, 2007-06, Vol.133 (6), p.2716-2729

2007

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SWIFT X-RAY OBSERVATIONS OF CLASSICAL NOVAE. II. THE SUPER SOFT SOURCE SAMPLE

The Astrophysical journal. Supplement series, 2011-12, Vol.197 (2), p.jQuery1323919417348='48'-jQuery1323919417348='48'

Schwarz, Greg J

2011

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ELEMENTAL ABUNDANCES IN THE EJECTA OF OLD CLASSICAL NOVAE FROM LATE-EPOCH SPITZER SPECTRA

The Astrophysical journal, 2012-08, Vol.755 (1), p.37-21

2012

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SOFIA/FORCAST Observations of R Aqr: Monitoring the Dust Emission

The Astrophysical journal, 2020-07, Vol.898 (1), p.31

2020

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Quenched Nitrogen-included Carbonaceous Composite (QNCC): A powerful candidate of the carriers of the UIR bands in classical novae

Proceedings of the International Astronomical Union, 2019-04, Vol.15 (S350), p.425-426

2019

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Nitrogen-included Carbonaceous Compounds (NCC): Laboratory-synthesized organics as the probable candidate for the carrier of the UIR bands observed in dusty classical novae

Proceedings of the International Astronomical Union, 2018-08, Vol.14 (S345), p.343-344

2018

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Photometric and Spectroscopic Analysis of Classical Novae: An Analysis of Their Observational Properties and Greater Astronomical Impact

Publications of the Astronomical Society of the Pacific, 2011-05, Vol.123 (903), p.645-647

Helton, L. Andrew

2011

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Searching for Cool Dust. II. Infrared Imaging of The OH/IR Supergiants, NML Cyg, VX Sgr, S Per, and the Normal Red Supergiants RS Per and T Per

The Astronomical journal, 2018-05, Vol.155 (5), p.212

2018

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The Unexpected Spectrum of the Innermost Ejecta of the Red Hypergiant VY CMa

Astrophysical journal. Letters, 2019-04, Vol.874 (2), p.L26

2019

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MASSIVE STAR FORMATION IN THE LMC. I. N159 AND N160 COMPLEXES

The Astrophysical journal, 2017-01, Vol.834 (2), p.122

2017

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The Dusty Nova V1065 Centauri (Nova Cen 2007): a Spectroscopic Analysis of Abundances and Dust Properties

The Astronomical journal, 2010-11, Vol.140 (5), p.1347-1369

2010

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Towards the identification of carriers of the unidentified infrared (UIR) bands in novae

Proceedings of the International Astronomical Union, 2020-11, Vol.16 (S366), p.327-331

2020

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The Three-Dimensional Morphology of VY Canis Majoris. II. Polarimetry and the Line-of-Sight Distribution of the Ejecta

The Astronomical journal, 2007-06, Vol.133 (6), p.2730-2736

2007

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Stellar Populations and Mass Loss in M15: A Spitzer Space Telescope Detection of Dust in the Intracluster Medium

The Astronomical journal, 2006-10, Vol.132 (4), p.1415-1425

2006

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THE SOFIA OBSERVATORY AT THE START OF ROUTINE SCIENCE OPERATIONS: MISSION CAPABILITIES AND PERFORMANCE

The Astrophysical journal. Supplement series, 2014-06, Vol.212 (2), p.1-13

2014

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SEARCHING FOR COOL DUST IN THE MID-TO-FAR INFRARED: THE MASS-LOSS HISTORIES OF THE HYPERGIANTS μ Cep, VY CMa, IRC+10420, AND ρ Cas

The Astronomical journal, 2016-03, Vol.151 (3), p.51

2016

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Searching for Cool Dust. II. Infrared Imaging of The OH/IR Supergiants, NML Cyg, VX Sgr, S Per, and the Normal Red Supergiants RS Per and T Per∗ ∗ Based on observations obtained with: (1) the NASA/DLR Stratospheric Observatory for Infrared Astronomy (SOFIA). SOFIA is jointly operated by the Universities Space Research Association, Inc. (USRA), under NASA contract NAS2-97001, and the Deutsches SOFIA Institut (DSI) under DLR contract 50 OK 0901 to the University of Stuttgart; and (2) the MMT Obser

The Astronomical journal, 2018-04, Vol.155 (5)

2018

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The Unexpected Spectrum of the Innermost Ejecta of the Red Hypergiant VY CMa∗ ∗ Based on observations made with the NASA/ESA Hubble Space Telescope, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555

Astrophysical journal. Letters, 2019-04, Vol.874 (2)

2019

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M33's Variable A: A Hypergiant Star More Than 35 YEARS in Eruption

The Astronomical journal, 2006-04, Vol.131 (4), p.2105-2113

2006

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SEARCHING FOR COOL DUST IN THE MID-TO-FAR INFRARED: THE MASS-LOSS HISTORIES OF THE HYPERGIANTS [mu] Cep, VY CMa, IRC+10420, AND [rho] Cas

The Astronomical journal, 2016-03, Vol.151 (3)

2016

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SEARCHING FOR COOL DUST IN THE MID-TO-FAR INFRARED: THE MASS-LOSS HISTORIES OF THE HYPERGIANTS Cep, VY CMa, IRC+10420, AND Cas Based on observations obtained with: (1) the NASA/DLR Stratospheric Observatory for Infrared Astronomy (SOFIA). SOFIA is jointly operated by the Universities Space Research Association, Inc. (USRA), under NASA contract NAS2-97001, and the Deutsches SOFIA Institut (DSI) under DLR contract 50 OK 0901 to the University of Stuttgart; and (2) the MMT Observatory on Mt. Hopkin

The Astronomical journal, 2016-02, Vol.151 (3)

2016

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The 3D morphology of the ejecta surrounding VY Canis Majoris

Proceedings of the International Astronomical Union, 2007-03, Vol.3 (S242), p.256-260

2007

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SN 2010U: A LUMINOUS NOVA IN NGC 4214

The Astrophysical journal, 2010, Vol.718 (1)

2010

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Nova V2362 Cygni (Nova Cygni 2006): Spitzer, Swift, and Ground-Based Spectral Evolution

The Astronomical journal, 2008-11, Vol.136 (5), p.1815-1827

2008

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On the Nature of Organic Dust in Novae

The Three-Dimensional Morphology of VY Canis Majoris. I. The Kinematics of the Ejecta

SWIFT X-RAY OBSERVATIONS OF CLASSICAL NOVAE. II. THE SUPER SOFT SOURCE SAMPLE

ELEMENTAL ABUNDANCES IN THE EJECTA OF OLD CLASSICAL NOVAE FROM LATE-EPOCH SPITZER SPECTRA

SOFIA/FORCAST Observations of R Aqr: Monitoring the Dust Emission

Quenched Nitrogen-included Carbonaceous Composite (QNCC): A powerful candidate of the carriers of the UIR bands in classical novae

Nitrogen-included Carbonaceous Compounds (NCC): Laboratory-synthesized organics as the probable candidate for the carrier of the UIR bands observed in dusty classical novae

Photometric and Spectroscopic Analysis of Classical Novae: An Analysis of Their Observational Properties and Greater Astronomical Impact

Searching for Cool Dust. II. Infrared Imaging of The OH/IR Supergiants, NML Cyg, VX Sgr, S Per, and the Normal Red Supergiants RS Per and T Per

The Unexpected Spectrum of the Innermost Ejecta of the Red Hypergiant VY CMa

MASSIVE STAR FORMATION IN THE LMC. I. N159 AND N160 COMPLEXES

The Dusty Nova V1065 Centauri (Nova Cen 2007): a Spectroscopic Analysis of Abundances and Dust Properties

Towards the identification of carriers of the unidentified infrared (UIR) bands in novae

The Three-Dimensional Morphology of VY Canis Majoris. II. Polarimetry and the Line-of-Sight Distribution of the Ejecta

Stellar Populations and Mass Loss in M15: A Spitzer Space Telescope Detection of Dust in the Intracluster Medium

THE SOFIA OBSERVATORY AT THE START OF ROUTINE SCIENCE OPERATIONS: MISSION CAPABILITIES AND PERFORMANCE

SEARCHING FOR COOL DUST IN THE MID-TO-FAR INFRARED: THE MASS-LOSS HISTORIES OF THE HYPERGIANTS μ Cep, VY CMa, IRC+10420, AND ρ Cas

The Unexpected Spectrum of the Innermost Ejecta of the Red Hypergiant VY CMa∗ ∗ Based on observations made with the NASA/ESA Hubble Space Telescope, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555

M33's Variable A: A Hypergiant Star More Than 35 YEARS in Eruption

SEARCHING FOR COOL DUST IN THE MID-TO-FAR INFRARED: THE MASS-LOSS HISTORIES OF THE HYPERGIANTS [mu] Cep, VY CMa, IRC+10420, AND [rho] Cas

The 3D morphology of the ejecta surrounding VY Canis Majoris

SN 2010U: A LUMINOUS NOVA IN NGC 4214

Nova V2362 Cygni (Nova Cygni 2006): Spitzer, Swift, and Ground-Based Spectral Evolution

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