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CAS95B - Methanol and hydroxyl maser positions

Short title: Caswell et al. (1995)
Authors: Caswell, J. L.Vaile, R. A.Forster, J. R.
Journal: Monthly Notices of the Royal Astronomical Society, Volume 277, Issue 1, pp. 210-216.
Bibcode:

Target type: Known_Class_II,OH
Transitions: OH_1665,CH3OH_6(II)

Abstract
The Australia Telescope Compact Array has been used to study more than 40 sites of 1.665-GHz hydroxyl masers and 36 sites of 6.668-GHz methanol masers. Maser positions accurate to better than 1 arcsec have been derived. At each maser site both species are commonly present, and comparisons have been made between the methanol and OH. In 28 of the 29 cases where we have accurate measurements of both species, the methanol and OH coincide to within the errors, with nominal separations of less than 1.4 arcsec. In only one case do the two species apparently arise from different sites, the separation in this instance exceeding 3 arcsec. 1.665-GHz OH masers are known to be excellent indicators of the sites of ultra-compact HII regions which envelop recently formed massive stars our results confirm with high accuracy that masers of 1.665-GHz OH and 6.6-GHz methanol generally pinpoint identical HII regions. Thus the same evolutionary phase of the HII region is conducive to both OH and methanol maser emission. We briefly discuss the precise distribution of the masing molecules relative to the embedded star and its HII region, but this requires further study.

Abstract

The Australia Telescope Compact Array has been used to study more than 40 sites of 1.665-GHz hydroxyl masers and 36 sites of 6.668-GHz methanol masers. Maser positions accurate to better than 1 arcsec have been derived. At each maser site both species are commonly present, and comparisons have been made between the methanol and OH. In 28 of the 29 cases where we have accurate measurements of both species, the methanol and OH coincide to within the errors, with nominal separations of less than 1.4 arcsec. In only one case do the two species apparently arise from different sites, the separation in this instance exceeding 3 arcsec. 1.665-GHz OH masers are known to be excellent indicators of the sites of ultra-compact HII regions which envelop recently formed massive stars our results confirm with high accuracy that masers of 1.665-GHz OH and 6.6-GHz methanol generally pinpoint identical HII regions. Thus the same evolutionary phase of the HII region is conducive to both OH and methanol maser emission. We briefly discuss the precise distribution of the masing molecules relative to the embedded star and its HII region, but this requires further study.

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Detection table from Caswell et al. (1995)

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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)
ATLASGAL 870 um	ATLASGAL 870 um + Planck	Bolocam 1.1 mm
UKIDSS K Download UKIDSS K FITS	2MASS K Download 2MASS K FITS

select MAX(oh_data_all.ra_hms) as ra_hms,MAX(oh_data_all.dec_dms) as dec_dms,MAX(oh_data_all.source_name) as source_name,MAX(oh_data_all.ra) as ra,MAX(oh_data_all.dec) as dec,MAX(oh_data_all.l) as l,MAX(oh_data_all.b) as b,MAX(oh_data_all.grp) as grp,MAX(oh_data_all.other_name) as other_name,MAX(oh_data_all.other_desc) as other_desc,BOOL_OR(thermal) as thermal,MAX(oh_data_all.freq) as freq,MAX(oh_data_all.vrange) as vrange,MAX(oh_data_all.vpeak) as vpeak,MAX(oh_data_all.peak) as peak,MAX(oh_data_all.fwhm) as fwhm,MAX(oh_data_all.int) as int,MAX(oh_data_all.rms) as rms,MAX(oh_data_all.units) as units,MAX(oh_data_all.units_rms) as units_rms,MAX(oh_data_all.date_txt) as date_txt,MAX(oh_data_all.telescope_ref) as telescope_ref,MAX(oh_data_all.telescope_conf) as telescope_conf,MAX(oh_data_all.v_step) as v_step,MAX(oh_data_all.beam) as beam,MAX(oh_data_all.beam_maj) as beam_maj,MAX(oh_data_all.beam_min) as beam_min,MAX(oh_data_all.beam_pa) as beam_pa,MAX(oh_data_all.ref) as ref,MAX(oh_data_all.list_ref) as list_ref,MAX(oh_data_all.ascii) as ascii,MAX(oh_data_all.image) as image,MAX(oh_data_all.descr) as descr,MAX(oh_data_all.id) as id,BOOL_OR(mjy_flag) as mjy_flag,BOOL_OR(rms_mjy_flag) as rms_mjy_flag,MAX(oh_data_all.dist) as dist,1 as dist_parallax,MAX(oh_data_all.date_txt) as date_txt,MAX(line_det) as line_det,MAX(type) as type,MAX(simbad_types_cat) as simbad_types_cat FROM oh_data_all  LEFT JOIN all_objects_withmet ON oh_data_all.grp=all_objects_withmet.group_name LEFT JOIN object_categories ON all_objects_withmet.group_name = object_categories.group_name_cat AND object_categories.tbl_cat = 'all_objects_withmet' LEFT JOIN transitions ON oh_data_all.line=transitions."Line"  WHERE ref ilike 'CAS95B' AND detected=true AND hide=false GROUP BY ref

select oh_data_all.ra_hms,oh_data_all.dec_dms,oh_data_all.source_name,oh_data_all.ra,oh_data_all.dec,oh_data_all.l,oh_data_all.b,oh_data_all.grp,oh_data_all.other_name,oh_data_all.other_desc,oh_data_all.thermal,oh_data_all.freq,oh_data_all.vrange,oh_data_all.vpeak,oh_data_all.peak,oh_data_all.fwhm,oh_data_all.int,oh_data_all.rms,oh_data_all.units,oh_data_all.units_rms,oh_data_all.date_txt,oh_data_all.telescope_ref,oh_data_all.telescope_conf,oh_data_all.v_step,oh_data_all.beam,oh_data_all.beam_maj,oh_data_all.beam_min,oh_data_all.beam_pa,oh_data_all.ref,oh_data_all.list_ref,oh_data_all.ascii,oh_data_all.image,oh_data_all.descr,oh_data_all.id,oh_data_all.mjy_flag,oh_data_all.rms_mjy_flag,oh_data_all.dist,oh_data_all.dist_parallax,oh_data_all.date_txt,line_det,type,simbad_types_cat FROM oh_data_all   LEFT JOIN all_objects_withmet ON oh_data_all.grp=all_objects_withmet.group_name LEFT JOIN object_categories ON all_objects_withmet.group_name = object_categories.group_name_cat AND object_categories.tbl_cat = 'all_objects_withmet' LEFT JOIN transitions ON oh_data_all.line=transitions."Line"  WHERE ref ilike 'CAS95B' AND detected=true AND hide=false ORDER BY detected DESC,id

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CAS95B - Methanol and hydroxyl maser positions

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Detection table from Caswell et al. (1995)