These tools will no longer be maintained as of December 31, 2024. Archived website can be found here. PubMed4Hh GitHub repository can be found here. Contact NLM Customer Service if you have questions.
8. Upper limits for the ethyl-cyanide abundances in TMC-1 and L134N: chemical implications. Minh YC; Irvine WM Astrophys Space Sci; 1991; 175():165-9. PubMed ID: 11538286 [TBL] [Abstract][Full Text] [Related]
9. Interstellar SiO as a tracer of high-temperature chemistry. Ziurys LM; Friberg P; Irvine WM Astrophys J; 1989 Aug; 343(1):201-7. PubMed ID: 11538345 [TBL] [Abstract][Full Text] [Related]
10. The composition of interstellar molecular clouds. Irvine WM Space Sci Rev; 1999; 90(1-2):203-18. PubMed ID: 11543287 [TBL] [Abstract][Full Text] [Related]
15. Chemical and physical gradients along the OMC-1 ridge. Ungerechts H; Bergin EA; Goldsmith PF; Irvine WM; Schloerb FP; Snell RL Astrophys J; 1997 Jun; 482(1 Pt 1):245-66. PubMed ID: 11541431 [TBL] [Abstract][Full Text] [Related]
16. Detection of nitric oxide in the dark cloud L134N. McGonagle D; Ziurys LM; Irvine WM; Minh YC Astrophys J; 1990 Aug; 359(1 Pt 1):121-4. PubMed ID: 11538685 [TBL] [Abstract][Full Text] [Related]
17. Chemical abundances in cold, dark interstellar clouds. Irvine WM; Ohishi M; Kaifu N Icarus; 1991 May; 91(1):2-6. PubMed ID: 11542208 [TBL] [Abstract][Full Text] [Related]
18. Are clouds collapsing at the 2' north position of Sagittarius B2? Minh YC; Haikala L; Hjalmarson A; Irvine WM Astrophys J; 1998 May; 498(1 Pt 1):261-6. PubMed ID: 11542936 [TBL] [Abstract][Full Text] [Related]