Y C Minh
Overview
Explore the profile of Y C Minh including associated specialties, affiliations and a list of published articles.
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Articles
18
Citations
17
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Recent Articles
11.
Minh Y, Irvine W
Astrophys Space Sci
. 1991 Jan;
175:165-9.
PMID: 11538286
We have sought interstellar ethyl-cyanide via its 2(02)-1(01) transition towards two cold, dark clouds and report upper limits of the total column densities of 3 x 10(12) cm-2 and 2...
12.
Minh Y, Brewer M, Irvine W, Friberg P, Johansson L
Astron Astrophys
. 1991 Jan;
244:470-6.
PMID: 11538285
We derive HOCO+ column densities approximately 10(15) cm-2 toward the Galactic center and < or = 10(12) cm-2 for cold dark clouds from observations and an LVG model. We mapped...
13.
Minh Y, Irvine W, Brewer M
Astron Astrophys
. 1991 Jan;
244:181-9.
PMID: 11538284
Several H2CS ortho and para transitions have been observed toward interstellar molecular clouds, including cold, dark clouds and star-forming regions. We derive H2CS fractional abundances f(H2CS) approximately 1-2 10(-9) relative...
14.
Minh Y, Ziurys L, Irvine W, McGonagle D
Astrophys J
. 1990 Sep;
360(1):136-41.
PMID: 11538684
Interstellar hydrogen sulfide (H2S) and its isotopic variant (H2(34)S) have been observed toward several positions in OMC-1 via their 1(10)-1(01) transitions near 168 GHz using the FCRAO 14 m telescope....
15.
McGonagle D, Ziurys L, Irvine W, Minh Y
Astrophys J
. 1990 Aug;
359(1 Pt 1):121-4.
PMID: 11538685
We report the first detection of interstellar nitric oxide (NO) in a cold dark cloud, L134N. Nitric oxide was observed by means of its two 2 pi 1/2, J =...
16.
Irvine W, Friberg P, Kaifu N, Matthews H, Minh Y, Ohishi M, et al.
Astron Astrophys
. 1990 Jan;
229:L9-12.
PMID: 11538681
We report the first detection of formic acid (HCOOH) in a cold, dark interstellar cloud (L134N). The observed abundance of 3x10(-10) relative to H2 is between one and two orders...
17.
Minh Y, Irvine W, Ziurys L
Astrophys J
. 1989 Oct;
345(1):L63-6.
PMID: 11538326
We have detected interstellar hydrogen sulfide (H2S) toward the cold, dark clouds L134N and TMC 1. We derive total column densities of approximately 2.6 x 10(13) cm-2 and approximately 7.0...
18.
Minh Y, Irvine W, Ziurys L
Astrophys J
. 1988 Nov;
334(1):175-81.
PMID: 11538465
A survey of the 4(04)-3(03) and 1(01)-0(00) transitions of HOCO+ has been made toward several molecular clouds. The HOCO+ molecule was not observed in any sources except Sgr B2 and...