activity
20082025
most citedNew Galactic supernova remnants discovered with IPHAS

69 citations · 257 across the 20 of their papers we have counts for

collaborators

20 papers

astro-ph.SR2025

Confirmation and characterization of Galactic planetary nebulae: insights from a spectroscopic study

D. A. Beleño-Molina, L. Olguín, L. F. Miranda +2

We present a spectroscopic investigation of 25 objects previously reported as possible Planetary Nebulae (PNe) in recent catalogs to obtain their physical properties and to establi…

astro-ph.SR2024★ 2 cited

Long and short term variability of the possible nascent planetary nebula IRAS 22568+6141: A late thermal pulse?

Roldán A. Cala, Luis F. Miranda, José F. Gómez +4

IRAS 22568+6141 has been classified as a low-ionisation planetary nebula (PN) and presents non-thermal radio continuum emission, which could be a signature of nascent PNe. We prese…

astro-ph.GA2024

Morphokinematical study of the planetary nebula Me2-1: Unveiling its point-symmetric and unusual physical structure

L. F. Miranda, R. Vázquez, L. Olguín +2

(Abridged) We present narrow-band images in several emission lines, and high- and intermediate-resolution long-slit spectra of Me2-1 to investigate its morphology and 3D structure,…

astro-ph.SR2023★ 7 cited

The origin of the planetary nebula M 1-16. A morphokinematic and chemical analysis

M. A. Gómez-Muñoz, R. Vázquez, L. Sabin +4

We investigated the origin of the Planetary Nebula (PN) M 1-16 using narrow-band optical imaging, and high- and low-resolution optical spectra to perform a detailed morpho-kinemati…

astro-ph.GA2021★ 2 cited

The reactivation of water maser emission in the planetary nebula IRAS 18061--2505 through a born-again episode

L. F. Miranda, O. Suárez, L. Olguín +12

Water maser emitting planetary nebulae (HO-PNe) are believed to be among the youngest PNe. We present new optical narrow- and broad-band images, intermediate- and high-resoluti…

astro-ph.SR2021★ 6 cited

The morpho-kinematical structure and chemical abundances of the complex planetary nebula NGC 1514

Alba Aller, Roberto Vázquez, Lorenzo Olguín +2

We present high-resolution, long-slit optical spectra and images of the planetary nebula NGC1514. The position velocity maps of the [OIII] emission line reveal complex kinematics w…

astro-ph.GA2019★ 3 cited

A Submillimeter Polarization Analysis of Frosty Leo

L. Sabin, Q. Zhang, R. Vázquez +1

We present a polarimetric investigation of the protoplanetary nebula Frosty Leo performed with the Submillimeter Array. We were able to detect, in the low continuum level (peak at…

astro-ph.SR2018★ 8 cited

Measuring the Expansion and Age of the Nova Shell IPHASXJ210204.7+471015

E. Santamaría, M. A. Guerrero, G. Ramos-Larios +4

The parallax expansion and kinematics of a nova shell can be used to assess its age and distance, and to investigate the interaction of the ejecta with the circumstellar medium. Th…

astro-ph.SR2018★ 12 cited

The interaction of the halo around the butterfly planetary nebula NGC650-1 with the interstellar medium

G. Ramos-Larios, M. A. Guerrero, A. Nigoche-Netro +7

With its bright and wide equatorial waist seen almost edge-on (the butterfly body) and the faint and broad bipolar extensions (the butterfly wings), NGC650-1 is the archetypical ex…

astro-ph.SR2017★ 9 cited

Catching a Grown-Up Starfish Planetary Nebula: I. Morpho-Kinematical study of PC 22

L. Sabin, M. A. Gómez-Muñoz, M. A. Guerrero +9

We present the first part of an investigation on the planetary nebula (PN) PC 22 which focuses on the use of deep imaging and high resolution echelle spectroscopy to perform a deta…

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.SR2015★ 13 cited

Millimeter polarisation of the protoplanetary nebula OH 231.8+4.2: A follow-up study with CARMA

L. Sabin, C. L. H. Hull, R. L. Plambeck +4

In order to investigate the characteristics and influence of the magnetic field in evolved stars, we performed a follow-up investigation of our previous submillimeter analysis of t…

astro-ph.SR2014★ 23 cited

The physical structure of planetary nebulae around sdO stars: Abell36, DeHt2, and RWT152

A. Aller, L. F. Miranda, L. Olguín +5

We present narrow-band Halpha and [OIII] images, and high-resolution, long-slit spectra of the planetary nebulae (PNe) Abell36, DeHt2, and RWT152 aimed at studying their morphology…

astro-ph.SR2013★ 20 cited

Submillimeter polarisation and magnetic field properties in the envelopes of proto-planetary nebulae CRL 618 and OH 231.8+4.2

L. Sabin, Q. Zhang, A. A. Zijlstra +5

We have carried out continuum and line polarisation observations of two Proto-planetary nebulae (PPNe), CRL 618 and OH 231.8+4.2, using the Submillimeter Array (SMA) in its compact…

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.SR2013★ 13 cited

Detection of a multi-shell planetary nebula around the hot subdwarf O-type star 2MASS J19310888+4324577

A. Aller, L. F. Miranda, A. Ulla +8

(Abridged) The origin of hot subdwarf O-type stars (sdOs) remains unclear since their discovery in 1947. Among others, a post-Asymptotic Giant Branch (post-AGB) origin is possible…

astro-ph.SR2013★ 69 cited

New Galactic supernova remnants discovered with IPHAS

L. Sabin, Q. A. Parker, M. E. Contreras +7

As part of a systematic search programme of a 10-degree wide strip of the Northern Galactic plane we present preliminary evidence for the discovery of four (and possibly five) new…

astro-ph.SR2012★ 19 cited

Bubbles and Knots in the Kinematical Structure of the Bipolar Planetary Nebula NGC 2818

Roberto Vázquez

High-resolution Hubble Space Telescope (HST) archive imaging and high-dispersion spectroscopy are used to study the complex morphological and kinematical structure of the planetary…

astro-ph.SR2010★ 7 cited

High Resolution Spectroscopy of the Planetary Nebulae PM1-242, PM1-318 and PM1-322

L. F. Miranda, R. Vázquez, M. A. Guerrero +2

We have recently confirmed the planetary nebula (PN)nature of PM1-242, PM1-318 and PM1-322. Here we present high-resolution long-slit spectra of these three PNe in order to analyze…

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…