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Planetary Nebulae

description587 papers
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lightbulbAbout this topic
Planetary nebulae are astronomical objects formed from the ejected outer layers of a dying star, typically a red giant, during the late stages of stellar evolution. They are characterized by a shell of ionized gas surrounding a central white dwarf, and they play a crucial role in the chemical enrichment of the interstellar medium.
lightbulbAbout this topic
Planetary nebulae are astronomical objects formed from the ejected outer layers of a dying star, typically a red giant, during the late stages of stellar evolution. They are characterized by a shell of ionized gas surrounding a central white dwarf, and they play a crucial role in the chemical enrichment of the interstellar medium.

Key research themes

1. How can the spectral classifications and physical characteristics of Central Stars of Planetary Nebulae (CSPNe) inform evolutionary pathways and binary influence in nebular formation?

This research theme focuses on compiling extensive spectroscopic data of CSPNe to analyze their spectral types, physical parameters (such as luminosity, temperature, and surface gravity), and binary fraction. Understanding these characteristics is crucial for interpreting the late stages of stellar evolution, the role of binary interactions in planetary nebula (PN) shaping, and the chemical diversity seen in PN populations. The availability of large, updated catalogues enables statistical validation of evolutionary models and addresses the relative prevalence of hydrogen-rich versus hydrogen-poor central stars, linking multiplicity to nebular morphology and composition.

Key finding: Compiled a new catalogue of 620 CSPNe with improved spectral classifications and physical data, increasing coverage by 25% over previous efforts. Found a hydrogen-rich to hydrogen-poor CSPNe ratio of approximately 2:1 and... Read more
Key finding: Utilized integral field and long-slit spectroscopy to reveal M 2-31's spatio-kinematic structure, identifying bipolar fast outflows aligned perpendicularly to a toroidal waist structure enclosing a [WC]-type... Read more
Key finding: Presented a decade-long collaborative effort led by amateur astronomers that contributed 209 spectroscopically confirmed Galactic PNe, representing ~5% of the known population. The discoveries, supported by spectral... Read more

2. How do the physical conditions, chemical abundances, and excitation mechanisms within planetary nebulae and their bipolar outflows elucidate nebular shaping and progenitor star characteristics?

This theme investigates the internal structure, spatial kinematics, and chemical composition of PNe, with special focus on bipolar morphologies and fast collimated outflows. Detailed spectroscopic and imaging studies resolve how nebular morphology relates to progenitor mass, chemical enrichment patterns, and dynamic interactions between fast winds and previously ejected material. Analyzing these aspects informs theories of nebular shaping, mass-loss histories, and the interplay between nucleosynthesis and nebular evolution.

Key finding: Identified and spectroscopically confirmed RCW 24 and RCW 69 as some of the nearest and largest evolved bipolar PNe, with enhanced nitrogen abundances and kinematics consistent with progenitors exceeding 2.0–2.5 M☉. Distances... Read more
Key finding: Through narrow-band optical and near-IR imaging and spectroscopy, demonstrated that Hu1-2 has typical Type I PN helium and nitrogen enrichment but unusually low abundances in oxygen, neon, sulfur, and argon. High-velocity... Read more

3. What role does ionization modeling and nebular emission play in understanding planetary nebulae structure, dust content, and late stellar evolution phenomena such as Late Thermal Pulses (LTP)?

This theme covers theoretical and observational modeling of nebular ionization structures, dust spatial distribution, and transient evolutionary stages (e.g., LTPs) that modify CSPN and nebular properties. It encompasses computational photoionization models, dust extinction mapping via Balmer lines, and evolutionary tracks pertaining to thermal pulses occurring post-AGB. Addressing these aspects advances the understanding of nebular emission diagnostic interpretation, dust effects on morphology and spectra, and evolutionary pathways explaining uncommon or rapidly changing PN central stars.

Key finding: Reviewed foundational and subsequent photoionization models accounting for hydrogen, helium, and heavy element ionization and temperature structures within PNe, emphasizing the importance of treating diffuse radiation... Read more
Key finding: Implemented a technique combining narrow-band Hα and Hβ imaging to obtain intrinsic dust extinction maps in 29 PNe, circumventing contamination by nebular continuum and temperature dependencies typical in infrared dust... Read more
Key finding: Presented stellar evolution models over a range of metallicities and masses demonstrating Late Thermal Pulse (LTP) phenomena characterized by helium flashes post-AGB departure causing rapid HR diagram looping. Showed that LTP... Read more

All papers in Planetary Nebulae

Se realizó el análisis del espectro de la nebulosa designada en el New General Catalog con el número 1501 (NGC1501), utilizando como herramienta de análisis el software Image Reduction and Analysis Facility (IRAF), con el cual se... more
A concise summary of the recent international workshop held in honour of the career of Agnès Acker is presented together with a brief exposition of her productive career in the study of Planetary Nebulae, the expelled, ionised outer... more
Over the past decade, the number of planetary nebula central stars (CSPN) known to exhibit the Wolf-Rayet (WR) phenomenon has grown substantially. Many of these discoveries have resulted from the Macquarie/AAO/Strasbourg Hα (MASH) PN... more
The detection of fullerene molecules in a variety of astrophysical environments suggests that smaller dehydrogenated carbon molecules may also be present in these sources. One of these is planar C24 which has been shown to be more stable... more
Motivated by the possible conflict between the Navarro-Frenk-White(NFW) model predictions for the dark matter contents of galactic systems and its correlation with baryonic surface density, we will explore an alternative paradigm for the... more
Symbiotic stars that are strong radio sources and have cool dust emitting in the infrared are expected to have extended emission nebulae around them. In order to search for such emission nebulae, we have carried out CCD imaging of three... more
We present an alternative for the description of galactic halos based on Tsallis' non-extensive entropy formalism; on this scheme, halos are stellar polytropes characterized by three parameters, the central density, ρ c , the central... more
We present 10 new Spitzer detections of fullerenes in Magellanic Cloud Planetary Nebulae, including the first extragalactic detections of the C 70 molecule. These new fullerene detections together with the most recent laboratory data... more
Abstract ……………………. ……………………………………………………………… Matter is programmed/designed according to the laws of the positive sciences: mathematics, physics, astrophysics, chemistry, and biology. These laws are translated into the extremely rich and... more