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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.
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: Table 1 and 2
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Detection table from Payne et al. (1988)
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Different Line detections
IRAS source
IRAS coordinates (RA, Dec)
IRAS source distance (arcsec)
IRAS flux density (F12,F25,F60,F100)
2MASS source
2MASS coordinates (RA, Dec)
2MASS source distance (arcsec)
2MASS magnituted (J,H,K)
GCVS source
GCVS coordinates (RA, Dec)
GCVS source distance (arcsec)
GCVS parameters
WISE source
WISE coordinates (RA, Dec)
WISE source distance (arcsec)
WISE magnitudes (w1, w2, w3, w4)
Akari IRC source
Akari IRC coordinates (RA, Dec)
Akari IRC source distance (arcsec)
Akari IRC fluxes (S09, S18)
Akari FIS source
Akari FIS coordinates (RA, Dec)
Akari FIS source distance (arcsec)
Akari FIS fluxes (S65, S90, S140, S160)
Continuum source
Continuum coordinates (RA, Dec)
Continuum source distance (arcsec)
Continuum parameters
Bolocam GPS
BGPS coordinates (RA, Dec)
BGPS source distance (arcsec)
BGPS parameters
EGO source
EGO coordinates (RA, Dec)
EGO source distance (arcsec)
EGO parameters
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PACS color (70-160 um)
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select MAX(oh_data.ra_hms) as ra_hms,MAX(oh_data.dec_dms) as dec_dms,MAX(oh_data.source_name) as source_name,MAX(oh_data.ra) as ra,MAX(oh_data.dec) as dec,MAX(oh_data.l) as l,MAX(oh_data.b) as b,MAX(oh_data.grp) as grp,MAX(oh_data.vlow) as vlow,MAX(oh_data.vup) as vup,MAX(oh_data.vpeak) as vpeak,MAX(oh_data.vpeak_e) as vpeak_e,MAX(oh_data.vpeak2) as vpeak2,MAX(oh_data.vpeak2_e) as vpeak2_e,MAX(oh_data.dv) as dv,MAX(oh_data.other_name) as other_name,MAX(oh_data.peak) as peak,MAX(oh_data.peak_e) as peak_e,MAX(oh_data.peak2) as peak2,MAX(oh_data.peak2_e) as peak2_e,MAX(oh_data.int) as int,MAX(oh_data.int_e) as int_e,MAX(oh_data.rms) as rms,MAX(oh_data.date) as date,MAX(oh_data.date2) as date2,MAX(oh_data.telescope_ref) as telescope_ref,MAX(oh_data.units) as units,MAX(oh_data.beam) as beam,MAX(oh_data.ref) as ref,MAX(oh_data.list_ref) as list_ref,MAX(oh_data.ascii) as ascii,MAX(oh_data.image) as image,MAX(oh_data.id) as id,MAX(oh_data.date_txt) as date_txt,MAX(oh_data.other_name) as other_name,MAX(oh_data.other_desc) as other_desc,BOOL_OR(thermal) as thermal,MAX(oh_data.line) as line,MAX(oh_data.vrange) as vrange,MAX(oh_data.vpeak) as vpeak,MAX(oh_data.peak) as peak,MAX(oh_data.fwhm) as fwhm,MAX(oh_data.int) as int,MAX(oh_data.rms) as rms,MAX(oh_data.units) as units,MAX(oh_data.units_rms) as units_rms,MAX(oh_data.date_txt) as date_txt,MAX(oh_data.telescope_ref) as telescope_ref,MAX(oh_data.beam) as beam,MAX(oh_data.beam_maj) as beam_maj,MAX(oh_data.beam_min) as beam_min,MAX(oh_data.beam_pa) as beam_pa,MAX(oh_data.ref) as ref,MAX(oh_data.list_ref) as list_ref,MAX(oh_data.ascii) as ascii,MAX(oh_data.image) as image,MAX(oh_data.descr) as descr,MAX(oh_data.id) as id,BOOL_OR(mjy_flag) as mjy_flag,BOOL_OR(rms_mjy_flag) as rms_mjy_flag,MAX(oh_data.dist) as dist,MAX(oh_data.date_txt) as date_txt,MAX(oh_data.freq) as freq,MAX(line_det) as line_det FROM oh_data LEFT JOIN all_objects_withmet ON oh_data.grp=all_objects_withmet.group_name WHERE ref ilike 'PAY88' AND detected=true AND hide=false GROUP BY ref
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.grp,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.date_txt,oh_data.other_name,oh_data.other_desc,oh_data.thermal,oh_data.line,oh_data.vrange,oh_data.vpeak,oh_data.peak,oh_data.fwhm,oh_data.int,oh_data.rms,oh_data.units,oh_data.units_rms,oh_data.date_txt,oh_data.telescope_ref,oh_data.beam,oh_data.beam_maj,oh_data.beam_min,oh_data.beam_pa,oh_data.ref,oh_data.list_ref,oh_data.ascii,oh_data.image,oh_data.descr,oh_data.id,oh_data.mjy_flag,oh_data.rms_mjy_flag,oh_data.dist,oh_data.date_txt,oh_data.freq,line_det FROM oh_data LEFT JOIN all_objects_withmet ON oh_data.grp=all_objects_withmet.group_name WHERE ref ilike 'PAY88' AND detected=true AND hide=false ORDER BY detected DESC,id
