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Data:
OH
PAY88 - A young planetary nebula with OH molecules - NGC 6302
Interferometry data
Short title
: Payne et al. (1988)
Authors
: Payne, H. E. Phillips, J. A. Terzian, Yervant
Journal
: Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 326, March 1, 1988, p. 368-375. Research supported by Cornell University.
Bibcode
:
1988ApJ...326..368P
Abstract
The results of a sensitive survey of planetary nebulae in all four ground-state OH lines are reported. The results confirm that evolved planetary nebulas are not OH sources in general. However, one interesting object was not detected: an OH 1612 MHz maser in the young planetary nebula NGC 6302. This nebula may be in a brief evolutionary stage, similar to the young and compact planetary nebula Vy 2-2, where OH has already been detected. In addition, the results of further observations of NGC 6302 are reported, including VLA observations of the 1612 MHz line and continuum emission and detections of rotationally excited OH lines at 5-cm wavelength in absorption.
Input tables
: Table 1 and 2
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Table (CSV)
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Detection table from Payne 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
17 13 44.4
-37 06 15.1
349.508004
1.055452
NGC 6302
1667
-54.4
-45.2
-54.4
-45.2
0.090
0.11
ENG15
PAY88
2
19 24 21.8
+09 53 55.7
45.497178
-2.70183
VY 2-2
1612
-62.0
-62.0
4.640
ENG15
PAY88
3
17 13 44.4
-37 06 15.1
349.508004
1.055452
NGC 6302
1612
-51.3
-40.5
-51.3
-40.5
0.140
0.55
ENG15
PAY88
Non-detection table from Payne et al. (1988)
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individual components
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)
Image size
:
arcsec (default is 120 arcsec)
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X
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 'PAY88' AND detected=true AND hide=false ORDER BY detected DESC,id
