Differences

This shows you the differences between two versions of the page.

--- molecules:ism:hydroxyaceton [2020/08/31 13:45] – mueller
+++ molecules:ism:hydroxyaceton [2026/03/04 11:30] (current) – mueller
@@ Line 3: / Line 3: @@
 Y. Zhou, D.-H. Quan, X. Zhang, and S.-L. Qin\\
 reported on the\\
-**[[https://doi.org/10.1088/1674–4527/20/8/125|Detection of Hydroxyacetone in Protostar IRAS 16293–2422 B]]**\\
+**[[https://doi.org/10.1088/1674-4527/20/8/125|Detection of Hydroxyacetone in Protostar IRAS 16293–2422 B]]**\\
 //Res. Astron. Astrophys.// **20**, (2020) Art. No. 125.\\
 The detection was made employing the ALMA Band 4 Science Verification data of IRAS 16293–2422 around 146 and 157 GHz. The number of unblended to moderately blended lines appears to be sufficient.\\
+\\
+In their work on\\
+**[[https://doi.org/10.1051/0004-6361/202558316|Expanding the C3H6O2 Isomeric Interstellar Inventory: Discovery of Lactaldehyde and Methoxyacetaldehyde in G+0.693−0.027]]**\\
+//Astron. Astrophys.// **706**, (2026) Art. No. A316.\\
+M. Sanz-Novo, V. M. Rivilla, I. Jiménez-Serra, L. Colzi, S. Zeng, A. Megías, D. San Andrés, Á. López-Gallifa, A. Martínez-Henares, Z. T. P. Fried, B. A. McGuire, S. Martín, M. A. Requena-Torres, B. Tercero, P. de Vicente, L. Kolesniková, E. R. Alonso, E. J. Cocinero, J. C. Guillemin, and I. Kleiner\\
+also report the detection of hydroxypropanone, also known as hydroxyacetone, in the course of a molecular line survey of this cold, shocked molecular cloud near Sagittarius B2 and in the Galactic center region. Several transitions with good signal-to-noise ratio (S/N) between 32 and 102 GHz were (essentially) unblended. The authors provide column density raios of the C<sub>3</sub>H<sub>6</sub>O<sub>2</sub> isomers.\\
+\\
 ----
-Contributor(s): H. S. P. Müller; 08, 2020
+Contributor(s): H. S. P. Müller; 08, 2020; 03, 2026
 ----