band 2 workshop nrao may 29, 2013 alma band 2: future prospects for scientific studies lucy m....
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![Page 1: Band 2 Workshop NRAO May 29, 2013 ALMA Band 2: Future Prospects for Scientific Studies Lucy M. Ziurys Staff and Students Arizona Radio Observatory University](https://reader037.vdocuments.us/reader037/viewer/2022110211/56649efc5503460f94c0ef65/html5/thumbnails/1.jpg)
Band 2 Workshop NRAO May 29, 2013
ALMA Band 2: Future Prospects for Scientific Studies
Lucy M. ZiurysStaff and Students
Arizona Radio ObservatoryUniversity of Arizona
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Band 2 Workshop NRAO May 29, 2013
“3 mm Low” at the ARO 12 m
• In 2000: Arizona took over the former NRAO 12 m at Kitt Peak
• 3 mm Low Receiver (65 – 88 GHz): Previous generation SIS mixers
• Used for many science projects over past 12.75 years
• Conducted MIC/MMIC test observations at ARO 12 m in spring 2013
ARO 12 m 3 mm Low receiver
Arizona
ObservatoryRadio
Arizona
ObservatoryRadio
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Band 2 Workshop NRAO May 29, 2013
Important Molecular TransitionsMolecule Frequency (GHz)
H2CO 10,1 → 00,0 72.84N2D+ J = 1→ 0 77.11HDO 11,0 →11,1 80.56HCP J = 2→ 1 79.90DCO+ J = 1→ 0 72.04DCN J = 1→ 0 72.41SiO J = 2→ 1 86.24
H13CO+ J = 1→ 0 86.75DNC J = 1→ 0 76.31NH2D 1+
1,1→ 1-0,1 85.92
SO 22→11 86.10HNO 10,1 →00,0 80.08
Importance of 67 – 90 GHz Region
• Many known spectral lines
• Unique physical and chemical tracers
• Contains fundamental transitions
of important molecules
• H2CO: Abundant molecule, excellent
thermometer and biologically relevant
• Deuterated Species: DCO+, N2D+,
DCN, HDO, NH2D
• HNO: Key species in N/O chemical
network
• J = 2→1 lines of SiO, SO, HCP:
Refractory and sulfur chemistry
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Band 2 Workshop NRAO May 29, 2013
• Deuterium: cosmological origin in universe (D/H ~ 10-5)
• Abundance not altered by star formation
• D/H ratio: Examine chemical fractionation in ion-molecule reactions
Significance of Deuterated Species in Band 2
++
++
• High D/H ratios found in molecular clouds
• Particularly high in COLD clouds
• Used to examine chemical pathways
• Tracer of cloud evolution
• J = 1→ 0 transition: very important
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Band 2 Workshop NRAO May 29, 2013
Refractory Chemistry
• SiO: Related to refractory material, dust grain evolution
• Also known to trace jet structures (HH212: Cabrit et. al. 2012)
• HCP: Phosphorus analog of HCN
• Only observed in circumstellar envelopes (Agundez et al.; Milam et al.)
•Tracer of phosphorus chemistry in dense clouds ?
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Band 2 Workshop NRAO May 29, 2013
New Molecules: Band 2
Zack, Halfen, & Ziurys, 2011, ApJ(Letters), 733, L36
TR
* (m
K)
VLSR (km s-1)
• Searching for new molecules
• Many blended/contaminated transitions
• Band 2 may provide critical and/or confirming lines
• Case for FeCN (First Fe-bearing species)
• 84 GHz transition (J = 10.5 → 9.5): essential for
identification
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Band 2 Workshop NRAO May 29, 2013
Ubiquitous H2CO• Excellent thermometer (multiple transitions)
• “Bio-marker”: Precursor to sugar Ribose
(RNA, DNA)
• Common molecule in molecular clouds
• Abundant in Outer Galaxy (DGC ~ 10 - 23 kpc)
• 72 GHz Transition FAVORABLE (101 → 000)
H2CO20.3 kpc
Blair et al. 2008
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Band 2 Workshop NRAO May 29, 2013
H2CO in Diffuse Clouds
• H2CO common in diffuse clouds
• Observed in absorption towards many site
lines (Liszt and Lucas 2003, 2006, etc.)
• Abundance H2CO/H2 ~ 4 x 10-9
• Factor of 5 less than cold molecular clouds
3C111
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Band 2 Workshop NRAO May 29, 2013
H2CO in Planetary Nebulae: Helix• Helix Nebula: one of oldest known PNe (~ 12, 000 yrs.)
• UV impinging on remnant shell material for some time
• H2CO widespread in Helix (Zack & Ziurys 2013)
• Abundance f (H2CO/H2)~ 0.3–2.1 × 10-7 Helix Nebula
~1000"
TK ~ 30 KN(H2) ~ 105 cm-3
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Band 2 Workshop NRAO May 29, 2013
~2’
H2CO in Red Spider Nebula• Red Spider (NGC 6537): Young PNe at 1,600 yrs
• Highest excitation planetary nebula known
• Presence of Si VI emission
• Interesting bipolar morphology
• H2CO present with f ~ 2 x 10-8 (relative to H2)
Edwards & Ziurys Ap.J. Letters, in press
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Band 2 Workshop NRAO May 29, 2013
SgrB2(N): Galactic Center
SgrB 2(N) at Band 2
1.5
1.0
0.5
0.0
TR
* (K
)
90x10385807570
Frequency (GHz)
• Spectrum: 68- 90 GHz: ARO 12 m data
• Part of SgrB2(N) survey in 1,2,3 mm windows
Halfen et al.
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Band 2 Workshop NRAO May 29, 2013
0.35
0.30
0.25
0.20
0.15
0.10
0.05
0.00
TR
* (K
)
74.6x10374.474.274.073.8
Frequency (GHz)
C2H
3CN
C2H
5CN
HC
OO
CH
3
HC
OO
CH
3
CH
3OC
H3
CH
3CN
v8=
1
+ C
H3C
N v
8=1
+ C
H3C
N v
8=1
HC
OO
CH
3C
H3C
N v
8=1
CH
3CN
v8=
1
CH
3OH
C2H
5CN HC
NH
+?
CH
3OC
H3
+ C
2H3C
N v
11=
1C
H3C
ON
H2 HC
OO
CH
3
HC
OO
CH
3
C2H
5OH
34S
O2
HC
5N
C2H5CN + U
U
UU
UUU
UUU
UUU
UU
• Fairly dense in lines at 10 mK level (SSB)
• Many organic-type species (C2H5CN, HCOOCH3,CH3OCH3, etc.)
• Also unidentified lines (“U”)
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Band 2 Workshop NRAO May 29, 2013
• Finished survey near 69 GHz as part of MIC testing
• Comparative 12 m data: 7. 7 hours integration
• POSITION SWITCHING: Off Position: 30‘ in AZ
• Frequency of 69.2 GHz (same relative T. scale)
SIS MIC
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Band 2 Workshop NRAO May 29, 2013
• Long integration at 72 GHz (H2CO): 31 hours
• Beam-switching towards IRC+10216
• Notice image contamination !!
SIS MIC
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Band 2 Workshop NRAO May 29, 2013
12 M Retirement: April 1, 2013
• But additional observations must wait…
• 12 m now retired
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Band 2 Workshop NRAO May 29, 2013
Speeches fromPast and CurrentDirectors…
Mark Gordon
Darrel Emerson
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Band 2 Workshop NRAO May 29, 2013
Final Blessing of the 12 mPaul Gabor, S.J.Vatican Observatory
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Band 2 Workshop NRAO May 29, 2013
Ceremonial Signing of the 12m Panel
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Band 2 Workshop NRAO May 29, 2013
A moment of silence as the compressors are turned off for the last time.
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Band 2 Workshop NRAO May 29, 2013
April 2, 2013: Work begins to dismantle old 12 m
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Band 2 Workshop NRAO May 29, 2013
Lift Elevation Axis, Yoke, Pedestal from Dome
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Band 2 Workshop NRAO May 29, 2013
Now outside dome with Tom Folkers
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Band 2 Workshop NRAO May 29, 2013
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Band 2 Workshop NRAO May 29, 2013
In Conclusion
• Observations have already shown Band 2 has much to offer scientifically
• 12 tests suggest use of MIC or MMIC may be acceptable instead of SIS
• NRAO-style (Kerr/Pan designs) SIS hard to beat
• Concerns about stability and image rejection with MMIC/MIC’s receivers
• Image rejection: properly-matched mixers in down-converter
• Further use of MIC and MMIC needed to draw concrete conclusions
• ARO will pursue Band 2 with new 12 m
• Next priority after installation of Band 3 receiver
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Band 2 Workshop NRAO May 29, 2013
ALMA Development FundNSF URO