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Data:
OH
SIV88 - Criteria for OH maser emission from circumstellar envelopes of oxygen-rich Mira-type red giants
Interferometry data
Short title
: Sivagnanam et al. (1988)
Authors
: Sivagnanam, P. Le Squeren, A. M. Foy, F.
Journal
: Astronomy and Astrophysics (ISSN 0004-6361), vol. 206, no. 2, Nov. 1988, p. 285-297.
Bibcode
:
1988A&A...206..285S
Abstract
A large and representative sample of oxygen-rich Mira stars was selected and observed in the 18 cm OH lines at their optical maximum. A total of 14 new OH sources were detected. The OH maser emission is found in the intrinsically bright far-IR objects with late M spectral type. Other characteristics of the Miras are high (H-K) and (K-L) colors. Their periods are on average longer and their (25-12) colors on average redder than those of non-OH Miras. The (J-H) and (60-25) colors are the same for OH and non-OH stars. In most cases, OH and H2O masers exist simultaneously. The observed stars form a sequence along which the period and the stellar luminosity increase, the stellar radius increases, the dust shell radius increases by a smaller factor, the photospheric temperature decreases but the dust shell temperature is roughly constant, and the mass loss rate and thus the thickness and the brighntess of the envelope increase considerably.
Comments:
Velocity resolution: 1.00 km/s
Upper limit for non-detections: 0.10 Jy (3σ)
Velocities and fluxes were determined from the spectra in Fig.1
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Table (CSV)
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Detection table from Sivagnanam et al. (1988)
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individual components
ID
Obs. RA
Obs. Dec
l
b
Source name
Frequency
V
low
V
up
V
peak
V
peak(2)
F
peak
F
peak(2)
List
Ref.
(J2000)
(J2000)
(deg.)
(deg.)
(MHz)
(km/s)
(km/s)
(km/s)
(km/s)
(Jy)
(Jy)
1
03 11 2.9
+14 47 58
166.141927
-36.101218
U Ari
1665
-56.5
-56.5
0.460
ENG15
SIV88
2
05 42 09
+32 02 24.1
176.964716
0.9902
U Aur
1665
2.0
11.0
2.0
11.0
0.290
0.25
ENG15
SIV88
3
05 42 09
+32 02 24.1
176.964716
0.9902
U Aur
1667
2.0
12.0
2.0
12.0
0.250
0.14
ENG15
SIV88
4
20 32 33.6
-21 41 26
22.942273
-31.445486
RU Cap
1612
3.5
9.5
3.5
9.5
0.330
0.44
ENG15
SIV88
5
20 32 33.6
-21 41 26
22.942273
-31.445486
RU Cap
1665
4.0
9.5
4.0
9.5
0.200
0.18
ENG15
SIV88
6
20 32 33.6
-21 41 26
22.942273
-31.445486
RU Cap
1667
4.0
10.0
4.0
10.0
0.190
0.22
ENG15
SIV88
7
13 51 25.5
-36 56 37.7
316.05722
24.39434
RX Cen
1665
7.0
7.0
0.090
ENG15
SIV88
8
13 51 25.5
-36 56 37.7
316.05722
24.39434
RX Cen
1667
-2.0
7.5
-2.0
7.5
0.190
0.14
ENG15
SIV88
9
05 46 56.3
-31 41 28.4
236.688826
-26.735245
S Col
1665
65.0
65.0
0.260
ENG15
SIV88
10
05 46 56.3
-31 41 28.4
236.688826
-26.735245
S Col
1667
65.0
65.0
0.370
ENG15
SIV88
11
16 10 14.5
+25 04 14.3
41.978001
45.61109
RU Her
1665
-15.5
-7.5
-15.5
-7.5
0.160
0.06
ENG15
SIV88
12
16 10 14.5
+25 04 14.3
41.978001
45.61109
RU Her
1667
-14.5
-8.0
-14.5
-8.0
0.180
0.13
ENG15
SIV88
13
06 37 31.3
-01 23 43.6
212.588003
-3.732456
SY Mon
1665
-55.0
-55.0
0.610
ENG15
SIV88
14
06 37 31.3
-01 23 43.6
212.588003
-3.732456
SY Mon
1667
-55.5
-55.5
0.240
ENG15
SIV88
15
05 29 0.9
-04 41 32.8
207.595954
-20.454978
S Ori
1665
-2.0
-2.0
0.360
ENG15
SIV88
16
22 12 16.2
+14 33 12.2
75.18579
-33.183332
RS Peg
1665
-24.5
-15.0
-24.5
-15.0
0.250
0.53
ENG15
SIV88
17
22 12 16.2
+14 33 12.2
75.18579
-33.183332
RS Peg
1667
-18.0
-18.0
0.160
ENG15
SIV88
18
17 53 48.8
-34 24 3.2
356.197227
-4.296947
SY Sco
1612
-13.5
-13.5
0.440
ENG15
SIV88
19
17 53 48.8
-34 24 3.2
356.197227
-4.296947
SY Sco
1665
-12.5
-12.5
0.170
ENG15
SIV88
20
17 07 35.8
-31 49 30
353.0245
5.196314
TU Sco
1665
-17.5
-17.5
0.130
ENG15
SIV88
21
17 07 35.8
-31 49 30
353.0245
5.196314
TU Sco
1667
-17.5
-17.5
0.130
ENG15
SIV88
22
14 17 19.9
+66 47 39.2
110.434496
48.196625
U Umi
1665
-8.5
-8.5
0.200
ENG15
SIV88
23
14 17 19.9
+66 47 39.2
110.434496
48.196625
U Umi
1667
-10.0
-10.0
0.140
ENG15
SIV88
24
08 16 33.8
+11 43 34.5
211.749441
24.139003
R Cnc
1665
11.8
11.8
3.910
ENG15
SIV88
25
18 38 21.1
+08 50 2.8
39.349682
6.904424
X Oph
1667
-55.2
-55.2
0.260
ENG15
SIV88
Non-detection table from Sivagnanam et al. (1988)
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Display associated data
Group name
Line detection (H
2
O, OH, SiO, CH
3
OH (I), CH
3
OH (II))
IRAS source
IRAS coordinates (RA, Dec)
IRAS flux density (F12,F25,F60,F100)
2MASS source
2MASS coordinates (RA, Dec)
2MASS magnituted (J,H,K)
Variable star
Variable star parameters
Star Formation Region name
Star Formation Region parameters
WISE source
WISE coordinates (RA, Dec)
WISE magnitudes (w1, w2, w3, w4)
Akari IRC source
Akari IRC coordinates (RA, Dec)
Akari IRC fluxes (S09, S18)
Akari FIS source
Akari FIS coordinates (RA, Dec)
Akari FIS fluxes (S65, S90, S140, S160)
Continuum
Continuum coordinates (RA, Dec)
Continuum parameters
Bolocam GPS
Bolocam coordinates (RA, Dec)
Bolocam parameters
Extended Green Objects
EGO coordinates (RA, Dec)
EGO parameters
View images
DSS (optical)
2MASS (JHK)
WISE (4-22 um)
IRAC (3-8 um)
GLIMPSE 360 (3.6-4.5 um)
PACS color (70-160 um)
SPIRE color (250-500 um)
AKARI color (60-160 um)
NVSS (1.4 GHz)
SDSS (optical+NIR)
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Position of H
2
O maser detection
DSS colored
2MASS colored
WISE colored
SDSS color
IRAC color I1,I2,I4
GLIMPSE 360
PACS color (70-160 um)
SPIRE color (250-500 um)
NVSS (1.4GHz)
UKIDSS K
2MASS K
select oh_data.ra_hms,oh_data.dec_dms,oh_data.source_name,oh_data.ra,oh_data.dec,oh_data.l,oh_data.b,oh_data.vlow,oh_data.vup,oh_data.vpeak,oh_data.vpeak_e,oh_data.vpeak2,oh_data.vpeak2_e,oh_data.dv,oh_data.other_name,oh_data.peak,oh_data.peak_e,oh_data.peak2,oh_data.peak2_e,oh_data.int,oh_data.int_e,oh_data.rms,oh_data.date,oh_data.date2,oh_data.telescope_ref,oh_data.units,oh_data.beam,oh_data.ref,oh_data.list_ref,oh_data.ascii,oh_data.image,oh_data.id,oh_data.freq FROM oh_data WHERE ref ilike 'SIV88' AND detected=true AND hide=false ORDER BY detected DESC,id
