activity
20132026
most citedProbing the Role of Carbon in the Interstellar Ultraviolet Extinction

47 citations · 99 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2026

Ultraviolet Interstellar Extinction toward High Galactic Latitudes

Ajay Mishra, Aigen Li

Nearby high Galactic latitude clouds provide a unique laboratory to study the physics and structure of the Galactic interstellar medium (ISM) and the properties of the interstellar…

astro-ph.GA2017★ 24 cited

Interstellar Silicon Depletion and the Ultraviolet Extinction

Ajay Mishra, Aigen Li

Spinning small silicate grains were recently invoked to account for the Galactic foreground anomalous microwave emission. These grains, if present, will absorb starlight in the far…

astro-ph.SR2016★ 14 cited

On the Relation between the Mysterious 21 Micrometer Emission Feature of Post-Asymptotic Giant Branch Stars and Their Mass Loss Rates

Ajay Mishra, Aigen Li, B. W. Jiang

Over two decades ago, a prominent, mysterious emission band peaking at ~20.1 micrometer was serendipitously detected in four preplanetary nebulae (PPNe; also known as "protoplaneta…

astro-ph.GA2015★ 47 cited

Probing the Role of Carbon in the Interstellar Ultraviolet Extinction

Ajay Mishra, Aigen Li

We probe the role of carbon in the ultraviolet (UV) extinction by examining the relations between the amount of carbon required to be locked up in dust [C/H]_dust with the 2175 Ang…

astro-ph.GA2015★ 11 cited

A Tale of Three Mysterious Spectral Features in Carbon-Rich Evolved Stars: The 21 Micrometer, 30 Micrometer, and "Unidentified Infrared" Emission Features

Ajay Mishra, Aigen Li, B. W. Jiang

The mysterious "21 micrometer" emission feature seen almost exclusively in the short-lived protoplanetary nebula (PPN) phase of stellar evolution remains unidentified since its dis…

astro-ph.SR2013★ 3 cited

Unidentified species in envelopes around carbon stars

Biwei Jiang, Aigen Li, Ke Zhang +3

The infrared (IR) spectra of many evolved carbon-rich stars exhibit two prominent dust emission features peaking around 21um and 30um, with the former exclusively seen in proto-pla…