The [NII] Line Ratio The ISO 122 m [NII] to SPIFI 205 m line ratio yields the density of the low ionization gas (Figure 5, blue line and circle)
Astronomy. H-R Diagram: Mapping the Stars by Luminosity and Surface Temperature Read! Pages 532-536.
Extra-Terrestrial Life and the Drake Equation Astronomy 311 Professor Lee Carkner Lecture 26.
Stellar Interiors Physical Astronomy Professor Lee Carkner Lecture 10.
Starbursts & Super Star Clusters J. Gallagher U. Wisconsin-Madison with L. J. Smith, M. Westmoquette (UCL), R. O’Connell (UVa), R. de Grijs (U. Sheffield)
This set of slides This set of slides starts the topic of stellar evolution, overview, protostars, main sequence… Units covered: 59, 60, 61.
Stages 12 – 14. Stage 12 – Low Mass Stars The carbon rich core continues to contract and heat up. Carbon fusion requires a temperature of 500 to 600 million.
Supernova!
The Evolution and Death of Stars 11/7 (Tuesday) Tailgate Party!! For Exam #3 4-6pm in RMN210 11/8 (Wednesday) Exam #3 HW # 8 – Stars – Due Wednesday the.
Star evolution
Star evolution Chapters 17 & 18 (Yes, we skip chap. 16, star birth)
The Disk-Jet Connection: A Universal Picture for Protostellar Jets Ralph Pudritz McMaster University Western Workshop: From Protostellar Disks to Planetary.
![The [NII] Line Ratio The ISO 122 m [NII] to SPIFI 205 m line ratio yields the density of the low ionization gas (Figure 5, blue line and circle)](https://static.fdocuments.us/doc/330x215/56649f465503460f94c68b56/the-nii-line-ratio-the-iso-122-m-nii-to-spifi-205-m-line-ratio.jpg)
