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

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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	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	15 44 11.1	-49 55 20	329.142434	3.949814	IRAS 15405-4945	1612	36.0	82.0	36.0	82.0	0.200	0.2	ENG15	LIN88
2	15 44 11.1	-49 55 20	329.142434	3.949814	IRAS 15405-4945	1665	36.0	64.0	36.0	64.0	0.500	2	ENG15	LIN88
3	15 44 11.1	-49 55 20	329.142434	3.949814	IRAS 15405-4945	1667	-17.0	70.0	-17.0	70.0	0.300	0.9	ENG15	LIN88
4	16 37 40	-38 20 17	344.073703	5.846602	IRAS 16342-3814	1612	-11.0	108.0	-11.0	108.0	1.000	8	ENG15	LIN88
5	16 37 40	-38 20 17	344.073703	5.846602	IRAS 16342-3814	1665	19.0	81.0	19.0	81.0	0.500	0.5	ENG15	LIN88
6	16 37 40	-38 20 17	344.073703	5.846602	IRAS 16342-3814	1667	-12.0	7.0	-12.0	7.0	0.300	0.5	ENG15	LIN88

Display associated data

Group name	Line detection (H₂O, OH, SiO, CH₃OH (I), CH₃OH (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

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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)
			Image size: arcsec (default is 120 arcsec)

Position of H₂O 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 '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

Interferometry data

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