Add to ORKGCO emission is a useful probe of the warm gas distribution in the planet forming regions of disks around Herbig Ae/Be (HAeBe) stars. We model UV fluoresced and thermally excited CO in the circumstellar disks of several HAeBes. We find indications of dust settling in the upper atmospheres of HD 141569 and HD 97048 and a correlation between PAH luminosity and gas heating in these two systems
We present high-resolution, near-infrared NIRSPEC observations of CO absorption toward six class II ...
This dissertation includes high-resolution, near-infrared spectroscopy to study CO in circumstellar ...
Context. CO rovibrational lines are efficient probes of warm molecular gas and can give unique insig...
CO is an important component of a protoplanetary disc as it is one of the most abundant gas phase ...
Aims: To calculate chemistry and gas temperature of evolving protoplanetary disks with decreasing ma...
Astronomy and Astrophysics 559 (2013): A84CO is an important component of a protoplanetary disc as i...
Author Institution: Department of Physics and Astronomy, University of Notre Dame; Institute for Ast...
Protoplanetary accretion disks are disks of dust and gas which surround and feed material onto a for...
CO is an important component of a protoplanetary disc as it is one of the most abundant gas phase sp...
We present a comparison of CO fundamental rovibrational lines (observed in the M band near 4.7 μm) f...
CO is an important component of a protoplanetary disc as it is one of the most abundant gas phase sp...
We present observations that indicate viscous heating contributes significantly to the surface heati...
Degree Awarded: Ph.D. Physics. The Catholic University of AmericaThis dissertation addresses several...
Artículo de publicación ISIAims. We study the emission and absorption of CO ro-vibrational lines in ...
We present a large, comprehensive survey of rovibrational CO line emission at 4.7 {$μ$}m from 69 p...
We present high-resolution, near-infrared NIRSPEC observations of CO absorption toward six class II ...
This dissertation includes high-resolution, near-infrared spectroscopy to study CO in circumstellar ...
Context. CO rovibrational lines are efficient probes of warm molecular gas and can give unique insig...
CO is an important component of a protoplanetary disc as it is one of the most abundant gas phase ...
Aims: To calculate chemistry and gas temperature of evolving protoplanetary disks with decreasing ma...
Astronomy and Astrophysics 559 (2013): A84CO is an important component of a protoplanetary disc as i...
Author Institution: Department of Physics and Astronomy, University of Notre Dame; Institute for Ast...
Protoplanetary accretion disks are disks of dust and gas which surround and feed material onto a for...
CO is an important component of a protoplanetary disc as it is one of the most abundant gas phase sp...
We present a comparison of CO fundamental rovibrational lines (observed in the M band near 4.7 μm) f...
CO is an important component of a protoplanetary disc as it is one of the most abundant gas phase sp...
We present observations that indicate viscous heating contributes significantly to the surface heati...
Degree Awarded: Ph.D. Physics. The Catholic University of AmericaThis dissertation addresses several...
Artículo de publicación ISIAims. We study the emission and absorption of CO ro-vibrational lines in ...
We present a large, comprehensive survey of rovibrational CO line emission at 4.7 {$μ$}m from 69 p...
We present high-resolution, near-infrared NIRSPEC observations of CO absorption toward six class II ...
This dissertation includes high-resolution, near-infrared spectroscopy to study CO in circumstellar ...
Context. CO rovibrational lines are efficient probes of warm molecular gas and can give unique insig...