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LIN88 - Two IRAS sources with high velocity outflow similar to OH231.8 + 4.2

Short title: te Lintel Hekkert et al. (1988)
Authors: te Lintel Hekkert, P. Habing, H. J. Caswell, J. L. Norris, R. P. Haynes, R. F.
Journal: Astronomy and Astrophysics (ISSN 0004-6361), vol. 202, no. 1-2, Aug. 1988, p. L19-L22.
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Abstract
In a search for OH maser emission from IRAS point sources the authors found amongst 700 detections two objects with exceptionally broad maser lines, between 150 and 200 km s^-1. They present their OH line data, IRAS data and some additional visual and near infrared information. It is suggested that the two objects, together with the well known object, OH 231.4+4.2 constitute a small group of OH/IR stars showing bipolar mass loss.	Comments: Velocity resolution: 1.00 km/s Entries taken from Table 1 or directly from the spectra.

Abstract

In a search for OH maser emission from IRAS point sources the authors found amongst 700 detections two objects with exceptionally broad maser lines, between 150 and 200 km s^-1. They present their OH line data, IRAS data and some additional visual and near infrared information. It is suggested that the two objects, together with the well known object, OH 231.4+4.2 constitute a small group of OH/IR stars showing bipolar mass loss.

Comments:
Velocity resolution: 1.00 km/s
Entries taken from Table 1 or directly from the spectra.

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Detection table from te Lintel Hekkert et al. (1988)

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ID	Obs. RA	Obs. Dec	l	b	Group id	Source name	Line	Frequency	V_range	V_peak	F_peak	List	Detection	Class	Dist. (parallax)	Ref.
	(J2000)	(J2000)	(deg.)	(deg.)			OH	(MHz)	(km/s)	(km/s)	(Jy)		Yes/No		(kpc)
1	15 44 11.1	-49 55 20	329.1424	3.9498	G329.142+3.950	IRAS 15405-4945	1612 MHz;	1612	46.0	36.0	0.200	ENG15	-CH₃OH II +OH	EVOLVED		LIN88
2	15 44 11.1	-49 55 20	329.1424	3.9498	G329.142+3.950	IRAS 15405-4945	1665 MHz;	1665	28.0	36.0	0.500	ENG15	-CH₃OH II +OH	EVOLVED		LIN88
3	15 44 11.1	-49 55 20	329.1424	3.9498	G329.142+3.950	IRAS 15405-4945	1667 MHz;	1667	87.0	-17.0	0.300	ENG15	-CH₃OH II +OH	EVOLVED		LIN88
4	16 37 40	-38 20 17	344.0737	5.8466	G344.074+5.847	IRAS 16342-3814	1612 MHz;	1612	119.0	-11.0	1.000	ENG15	+H₂O +OH -SiO	EVOLVED		LIN88
5	16 37 40	-38 20 17	344.0737	5.8466	G344.074+5.847	IRAS 16342-3814	1665 MHz;	1665	62.0	19.0	0.500	ENG15	+H₂O +OH -SiO	EVOLVED		LIN88
6	16 37 40	-38 20 17	344.0737	5.8466	G344.074+5.847	IRAS 16342-3814	1667 MHz;	1667	19.0	-12.0	0.300	ENG15	+H₂O +OH -SiO	EVOLVED		LIN88

DSS colored	2MASS colored	WISE colored
PACS color (70-160 um)	SPIRE color (250-500 um)	GLIMPSE 360
SDSS color	IRAC color I1,I2,I4	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.line) as line,MAX(oh_data_all.freq) as freq,MAX(oh_data_all.pol) as pol,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.url) as url,MAX(oh_data_all.image) as image,MAX(oh_data_all.image2) as image2,MAX(oh_data_all.image3) as image3,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 'LIN88' 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.line,oh_data_all.freq,oh_data_all.pol,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.url,oh_data_all.image,oh_data_all.image2,oh_data_all.image3,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 'LIN88' AND detected=true AND hide=false ORDER BY detected DESC,id

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LIN88 - Two IRAS sources with high velocity outflow similar to OH231.8 + 4.2

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Detection table from te Lintel Hekkert et al. (1988)