activity
20002015
most citedResolving the CO Snow Line in the Disk around HD 163296

123 citations · 198 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2015★ 10 cited

Morpho-kinematics of the planetary nebula NGC 3242: an analysis beyond its multiple-shell structure

M. A. Gómez-Muñoz, M. W. Blanco Cárdenas, R. Vázquez +3

In this paper we present the results of optical high-resolution imaging and spectroscopy of the complex planetary nebula (PN) NGC~3242. Our study is based on the analysis of the na…

astro-ph.GA2013★ 15 cited

Multiple outflows in the planetary nebula NGC 6058

P. F. Guillén, R. Vázquez, L. F. Miranda +4

We present narrow-band [O III]lambda5007 and H-alpha images, as well as long-slit high-resolution echelle spectra of the planetary nebula NGC 6058. Our data reveal that NGC 6058 is…

astro-ph.SR2011★ 123 cited

Resolving the CO Snow Line in the Disk around HD 163296

Chunhua Qi, Paola D'Alessio, Karin I. Oberg +4

We report Submillimeter Array (SMA) observations of CO (J=2--1, 3--2 and 6--5) and its isotopologues (13CO J=2--1, C18O J=2--1 and C17O J=3--2) in the disk around the Herbig Ae sta…

astro-ph.SR2010★ 10 cited

Observational Study of the Multistructured Planetary Nebula NGC 7354

M. E. Contreras, R. Vázquez, L. F. Miranda +3

We present an observational study of the planetary nebula (PN) NGC 7354 consisting of narrowband Halpha and [NII]6584 imaging as well as low- and high-dispersion long-slit spectros…

astro-ph2008★ 19 cited

The physical structure of the point-symmetric and quadrupolar planetary nebula NGC 6309

R. Vázquez, L. F. Miranda, L. Olguín +4

We analyse the point-symmetric planetary nebula NGC 6309 in terms of its three-dimensional structure and of internal variations of the physical conditions to deduce the physical pr…

astro-ph2000★ 21 cited

Optical and Near Infrared Study of the Cepheus E outflow, a very low excitation object

S. Ayala, A. Noriega-Crespo, P. M. Garnavich +4

We present images and spectra of the Cepheus E (Cep E) region at both optical and infrared wavelengths. Only the brightest region of the southern lobe of the Cep E outflow reveals…