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| More recently, two transition with complex velocity components have been detected in the centimeter range toward Sgr B2(N-LMH) employing the GBT:\\ | More recently, two transition with complex velocity components have been detected in the centimeter range toward Sgr B2(N-LMH) employing the GBT:\\ | ||
| J. M. Hollis,\\ | J. M. Hollis,\\ | ||
| - | **[[hollis_asilomar.pdf|Complex Molecules and the GBT: Is Isomerism the Key ?]]**,\\ | + | **{{ :pdfs:hollis_asilomar.pdf |Complex Molecules and the GBT: Is Isomerism the Key ?}}**, |
| Contribution at the IAU Symposium 231, Astrochemistry throughout the Universe, Asilomar, CA.\\ | Contribution at the IAU Symposium 231, Astrochemistry throughout the Universe, Asilomar, CA.\\ | ||
| While it is hard to say that the detection is beyond doubt, these two lines render the detection quite secure – mainly because the line density at these lower frequencies is fairly small. | While it is hard to say that the detection is beyond doubt, these two lines render the detection quite secure – mainly because the line density at these lower frequencies is fairly small. | ||