activity
20122019
most citedMid-IR Spectra of Type Ia SN 2014J in M82 Spanning the First Four Months

49 citations · 212 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.SR2019

Polarization in Disks

Ian Stephens, Zhi-Yun Li, Haifeng Yang +24

Polarized dust emission outside of disks reveal the magnetic field morphology of molecular clouds. Within disks, however, polarized dust emission can arise from very different mech…

astro-ph.GA2018★ 5 cited

Gemini, SOFIA, and ATCA Reveal Very Young, Massive Protostars in the Collapsing Molecular Cloud BYF 73

Rebecca L. Pitts, Peter J. Barnes, Stuart D. Ryder +1

We present multi-wavelength data on the globally infalling molecular cloud/protostellar cluster BYF 73. These include new far-IR spectral line and continuum data from SOFIA's Far I…

astro-ph.SR2018★ 16 cited

Herschel PACS observations of 4-10 Myr old Classical T Tauri stars in Orion OB1

Karina Maucó, César Briceño, Nuria Calvet +12

We present \emph{Herschel} PACS observations of 8 Classical T Tauri Stars in the Myr old OB1a and the Myr old OB1b Orion sub-asscociations. Detailed modeling…

astro-ph.IM2017★ 11 cited

Temporal Variations of Telluric Water Vapor Absorption at Apache Point Observatory

Dan Li, Cullen H. Blake, David Nidever +1

Time-variable absorption by water vapor in Earth's atmosphere presents an important source of systematic error for a wide range of ground-based astronomical measurements, particula…

astro-ph.EP2017★ 15 cited

Mid-Infrared Polarization of Herbig Ae/Be Discs

Dan Li, Charles M. Telesco, Han Zhang +4

We measured mid-infrared polarization of protoplanetary discs to gain new insight into their magnetic fields. Using CanariCam at the 10.4 m Gran Telescopio Canarias, we detected li…

astro-ph.GA2017★ 14 cited

Detection of Polarized Infrared Emission by Polycyclic Aromatic Hydrocarbons in the MWC 1080 Nebula

Han Zhang, Charles M. Telesco, Thiem Hoang +5

Polycyclic aromatic hydrocarbons (PAHs) are ubiquitous in astrophysical environments, as revealed by their pronounced emission features at 3.3, 6.2, 7.7, 8.6, 11.3, and 12.7 m c…