activity
20122018
most citedSPIRITS: Uncovering Unusual Infrared Transients With Spitzer

102 citations · 376 across the 14 of their papers we have counts for

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Showing astro-ph.SRShow all

11 papers · 1 filter

astro-ph.SR2018★ 5 cited

SOFIA/FORCAST Observations of the Luminous Blue Variable Candidates MN 90 and HD 168625

Ryan Arneson, Dinesh Shenoy, Nathan Smith +1

We present SOFIA/FORCAST imaging of the circumstellar dust shells surrounding the luminous blue variable (LBV) candidates MN 90 and HD 168625 to quantify the mineral abundances of…

astro-ph.SR2018★ 35 cited

The Temporal Development of Dust Formation and Destruction in Nova Sagittarii 2015#2 (V5668 Sgr): A Panchromatic Study

R. D. Gehrz, A. Evans, C. E. Woodward +15

We present 5-28 micron SOFIA FORECAST spectroscopy complemented by panchromatic X-ray through infrared observations of the CO nova V5668 Sgr documenting the formation and destructi…

astro-ph.SR2017★ 18 cited

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

Michael S. Gordon, Roberta M. Humphreys, Terry J. Jones +6

New MMT/MIRAC (9-11 μm), SOFIA/FORCAST (11-37 μm), and Herschel/PACS (70 and 160 μm) infrared (IR) imaging and photometry is presented for three famous OH/IR red supergiants (NML C…

astro-ph.SR2017★ 5 cited

A SOFIA FORCAST Grism Study of the Mineralogy of Dust in the Winds of Proto-planetary Nebulae: RV Tauri Stars and SRd Variables

R. A. Arneson, R. D. Gehrz, C. E. Woodward +10

We present a SOFIA FORCAST grism spectroscopic survey to examine the mineralogy of the circumstellar dust in a sample of post-asymptotic giant branch yellow supergiants that are be…

astro-ph.SR2016★ 29 cited

Rise and fall of the dust shell of the classical nova V339 Delphini

A. Evans, D. P. K. Banerjee, R. D. Gehrz +16

We present infrared spectroscopy of the classical nova V339 Delphini, obtained over a year period. The infrared emission lines were initially symmetrical, with HWHM velocit…

astro-ph.SR2015★ 62 cited

Searching for Cool Dust in the Mid-to-Far Infrared: the Mass Loss Histories of The Hypergiants Cep, VY CMa, IRC+10420, and Cas

Dinesh Shenoy, Roberta M. Humphreys, Terry Jay Jones +6

We present mid- and far- IR imaging of four famous hypergiant stars: the red supergiants Cep and VY CMa, and the warm hypergiants IRC +10420 and Cas. Our 11 to 37 m SOFI…

astro-ph.SR2015★ 1 cited

Panchromatic imaging and spectroscopic observations of the mass ejections of RY Scuti

Robert D. Gehrz, Nathan Smith, Dinesh Shenoy

We describe recent panchromatic imaging and spectroscopic studies of the supergiant, mass-transferring, binary star RY Scuti, which is in a brief transitional phase to become a Wol…

astro-ph.SR2015

Probing Hypergiant Mass Loss with Adaptive Optics Imaging & Polarimetry in the Infrared: MMT-Pol and LMIRCam observations of IRC +10420 & VY Canis Majoris

Dinesh P. Shenoy, Terry J. Jones, Chris Packham +1

We present 2 - 5 micron adaptive optics (AO) imaging and polarimetry of the famous hypergiant stars IRC +10420 and VY Canis Majoris. The imaging polarimetry of IRC +10420 with MMT-…

astro-ph.SR2015★ 19 cited

Observations of Type Ia Supernova 2014J with FLITECAM/SOFIA

William D. Vacca, Ryan T. Hamilton, Maureen Savage +9

We present medium resolution near-infrared (NIR) spectra, covering 1.1 to 3.4 microns, of the normal Type Ia supernova (SN Ia) SN 2014J in M82 obtained with the FLITECAM instrument…

astro-ph.SR2013★ 23 cited

Adaptive Optics Imaging of VY Canis Majoris at 2 - 5 micron with LBT/LMIRCam

Dinesh P. Shenoy, Terry J. Jones, Roberta M. Humphreys +11

We present adaptive optics images of the extreme red supergiant VY Canis Majoris in the Ks, L' and M bands (2.15 to 4.8 micron) made with LMIRCam on the Large Binocular Telescope (…

astro-ph.SR2012★ 32 cited

Elemental Abundances in the Ejecta of Old Classical Novae from Late-Epoch Spitzer Spectra

L. Andrew Helton, Robert D. Gehrz, Charles E. Woodward +7

We present Spitzer Space Telescope mid-infrared IRS spectra, supplemented by ground-based optical observations, of the classical novae V1974 Cyg, V382 Vel, and V1494 Aql more than…