Dust around AFGL 2688, molecular shielding, and the production of carbon chain molecules
                            Journal Article
                            ·
                            
                            · Astrophysical Journal; (USA)
                            
                        
                    - California Univ., Los Angeles (USA)
The molecular, IR, and optical maps of the evolved carbon star AFGL 2688 (the Egg Nebula) are all consistent with a model of a bipolar outflow of approximately 0.0001 solar masses/yr that stopped as this object evolved beyond the asymptotic giant branch about 200 years ago. In order to explain the extended HC7N emission around this star, it is proposed that carbon grains are collisionally fragmented as they supersonically steam through the circumstellar envelope. 60 refs.
- OSTI ID:
- 6851834
- Journal Information:
- Astrophysical Journal; (USA), Journal Name: Astrophysical Journal; (USA) Vol. 351; ISSN ASJOA; ISSN 0004-637X
- Country of Publication:
- United States
- Language:
- English
Similar Records
                                
                                
                                    
                                        
                                        Neutral carbon in the EGG nebula (AFGL 2688)
                                        
A MOLECULAR LINE SURVEY OF THE CARBON-RICH PROTOPLANETARY NEBULA AFGL 2688 IN THE 3 mm AND 1.3 mm WINDOWS
CRL 2688 and CRL 618: Proto--planetary nebulae
                        
                                            Journal Article
                                            ·
                                            Sat Oct 15 00:00:00 EDT 1983
                                            · Astrophys. J.; (United States)
                                            ·
                                            OSTI ID:6741975
                                        
                                        
                                        
                                    
                                
                                    
                                        A MOLECULAR LINE SURVEY OF THE CARBON-RICH PROTOPLANETARY NEBULA AFGL 2688 IN THE 3 mm AND 1.3 mm WINDOWS
                                            Journal Article
                                            ·
                                            Sat Aug 10 00:00:00 EDT 2013
                                            · Astrophysical Journal
                                            ·
                                            OSTI ID:22131046
                                        
                                        
                                        
                                    
                                
                                    
                                        CRL 2688 and CRL 618: Proto--planetary nebulae
                                            Journal Article
                                            ·
                                            Wed Mar 31 23:00:00 EST 1976
                                            · Astrophys. J., Lett.; (United States)
                                            ·
                                            OSTI ID:7346158
                                        
                                        
                                        
                                    
                                
                            Related Subjects
                                
                                    
                                        
                                        
                                            
                                                640102* -- Astrophysics & Cosmology-- Stars & Quasi-Stellar
Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
CARBON STARS
CHEMISTRY
COSMIC DUST
COSMOCHEMISTRY
CYANIDES
DISSOCIATION
DUSTS
HYDROGEN COMPOUNDS
MAIN SEQUENCE STARS
MAPS
MASS
MASS TRANSFER
MATHEMATICAL MODELS
NEBULAE
PLANETARY NEBULAE
STAR EVOLUTION
STAR MODELS
STARS
                                            
                                        
                                    
                                
                            
                        Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
CARBON STARS
CHEMISTRY
COSMIC DUST
COSMOCHEMISTRY
CYANIDES
DISSOCIATION
DUSTS
HYDROGEN COMPOUNDS
MAIN SEQUENCE STARS
MAPS
MASS
MASS TRANSFER
MATHEMATICAL MODELS
NEBULAE
PLANETARY NEBULAE
STAR EVOLUTION
STAR MODELS
STARS