J. Ricardo Rizzo

Dr. J. Ricardo Rizzo

Astrophysics and Space Sciences, ISDEFE, Madrid, Spain
orcid
Radio Astronomy - Archives - Open for collaborations

Research Focus & Metrics

Academic Career Length

29Years (1998-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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14 January 2005 in The Astrophysical Journal
Verified
Journal Article
Closed access
AFA. Fuente
A. Fuente
SGS. García-Burillo
S. García-Burillo
MGM. Gerin
M. Gerin
DTD. Teyssier
D. Teyssier
AUA. Usero
A. Usero
PVP. de Vicente
P. de Vicente
The nucleus of M82 has been mapped in several 3mm and 1mm lines of CN, HCN, C2H, c-C3H2, CH3C2H, HC3N and HOC+ using the IRAM 30m telescope. These species have been purposely selected as good tracers of photon-dominated chemistry. We have measured [CN]/[HCN] ~ 5 in the inner 650 pc galaxy disk. Furthermore, we have detected the HOC+ 1--0 line with an intensity similar to that of the H13CO+ 1--0 line. This implies a [HCO+]/[HOC+] ratio of ~40. These results corroborate the existence of a giant photo-dissociation region (PDR) in the nucleus of M82. In fact, the low [HCO+]/[HOC+] ratio can only be explained if the nucleus of M82 is formed by small (r<0.02-0.2 pc) and dense (n ~ a few 10^4--10^5 cm^{-3}) clouds immersed in an intense UV field (G_0 ~ 10^4 in units of the Habing field). The detection of the hydrocarbons c-C3H2 and CH3C2H in the nucleus of M82 suggests that a complex carbon chemistry is developing in this giant PDR.

10 February 2001 in The Astrophysical Journal
Verified
Journal Article
Open access
PDF file
JMJ. Martín-Pintado
J. Martín-Pintado
J. Ricardo RizzoJ. Ricardo Rizzo
J. Ricardo Rizzo
PVP. de Vicente
P. de Vicente
Nemesio Rodriguez-FernandezNemesio Rodriguez-Fernandez
Nemesio Rodriguez-Fernandez
AFA. Fuente
A. Fuente
We present observations of C2H5OH toward molecular clouds in Sgr A, Sgr B2 and associated with thermal and non-thermal features in the Galactic center. C2H5OH emission in Sgr A and Sgr B2 is widespread, but not uniform. C2H5OH emission is much weaker or it is not detected in some molecular clouds in both complexes, in particular those with radial velocities between 70 and 120 km/s. While most of the clouds associated with the thermal features do not show C2H5OH emission, that associated with the Non-Thermal Radio Arc shows emission. The fractional abundance of C2H5OH in most of the clouds with radial velocities between 0 and 70 km/s in Sgr A and Sgr B2 is relatively high, of few 1e-8. The C2H5OH abundance decreases by more than one order of magnitude (aprox. 1e-9) in the clouds associated with the thermal features. The large abundance of C2H5OH in the gas-phase indicates that C2H5OH has formed in grains and released to gas-phase by shocks in the last aprox. 1e5 years.Comment: In press in Astrophysical Journal Letters 7 pages, 1 table, 1 figur

21 June 2012 in Astronomy & Astrophysics
Verified
Journal Article
Open access
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DGD. Ginard
D. Ginard
MGM. González-García
M. González-García
AFA. Fuente
A. Fuente
JCJ. Cernicharo
J. Cernicharo
TAT. Alonso-Albi
T. Alonso-Albi
CJC. Joblin
C. Joblin
Astronomy & Astrophysics (A&A) is an international journal which publishes papers on all aspects of astronomy and astrophysics

6 November 2008 in Astronomy & Astrophysics
Verified
Journal Article
Open access
PDF file
AFA. Fuente
A. Fuente
SGS. García-Burillo
S. García-Burillo
AUA. Usero
A. Usero
MGM. Gerin
M. Gerin
RNR. Neri
R. Neri
JTJonathan Tennyson
Jonathan Tennyson
Astronomy & Astrophysics (A&A) is an international journal which publishes papers on all aspects of astronomy and astrophysics

1 June 2010 in Astronomy & Astrophysics
Verified
Journal Article
Open access
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NCN. Crimier
N. Crimier
CCC. Ceccarelli
C. Ceccarelli
TAT. Alonso-Albi
T. Alonso-Albi
AFA. Fuente
A. Fuente
PCP. Caselli
P. Caselli
FWF. Wyrowski
F. Wyrowski
Astronomy & Astrophysics (A&A) is an international journal which publishes papers on all aspects of astronomy and astrophysics

1 January 2020 in Advances In Space Research
Verified
Journal Article
Open access
YKYuri Kovalev
Yuri Kovalev
NKN.S. Kardashev
N.S. Kardashev
KSK.V. Sokolovsky
K.V. Sokolovsky
PVP.A. Voitsik
P.A. Voitsik
TATao An
Tao An
VZV.A. Zuga
V.A. Zuga