Search
References
Objects
Download
Papers & Acknowledgement
☰
Display data from paper
Data:
OH
LIN91B - An OH survey of very cold IRAS point sources
Interferometry data
Short title
: te Lintel Hekkert (1991B)
Authors
: te Lintel Hekkert, P.
Journal
: Astronomy and Astrophysics (ISSN 0004-6361), vol. 248, no. 1, Aug. 1991, p. 209-220.
Bibcode
:
1991A&A...248..209T
Abstract
A radio telescope survey of 84 IRAS point sources was carried out at all four 18-cm transitions of the OH radical in order to find protoplanetary nebulae (PPN). Emission or absorption was detected from 13 sources. Of these, nine are compact H II regions or star formation regions and four are PPN. High angular resolution observations of both H II regions and PPN are needed to provide information on the geometry and dynamics of the dust and gas envelope.
Target sources:
IRAS
Comments:
Velocity resolution: 0.90 km/s
Upper limit for non-detections: 0.3 Jy (3σ)
Among the detected sources only ""PPN"" are included. The majority of observed and undetected sources probably belong to star-forming regions.
Input tables
: Table 2 and 3
Download as
:
Table (CSV)
View paper statistics
Detection table from te Lintel Hekkert (1991B)
Export table to csv
Hide
/
Show
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 45 14.1
-17 56 47
9.364063
5.778882
IRAS 17423-1755
1667
21.5
46.0
21.5
46.0
0.300
0.7
ENG15
LIN91B
2
18 30 30.8
-14 28 58
17.684101
-2.032782
IRAS 18276-1431
1612
48.4
72.8
48.4
72.8
72.200
76.7
ENG15
LIN91B
3
18 30 30.8
-14 28 58
17.684101
-2.032782
IRAS 18276-1431
1667
47.9
74.6
47.9
74.6
0.400
1.2
ENG15
LIN91B
4
18 51 46.8
-02 04 09
31.129172
-1.019416
IRAS 18491-0207
1667
60.0
60.0
0.600
ENG15
LIN91B
5
22 05 30.5
+53 21 33
99.633809
-1.835619
IRAS 22036+5306
1612
-65.6
-16.6
-65.6
-16.6
0.700
0.7
ENG15
LIN91B
6
22 05 30.5
+53 21 33
99.633809
-1.835619
IRAS 22036+5306
1667
-68.0
-68.0
0.500
ENG15
LIN91B
Non-detection table from te Lintel Hekkert (1991B)
Export table to csv
Hide
/
Show
individual components
Display associated data
Group name
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
Select all
Select all
Select all
Select all
View images
DSS (optical)
SDSS (optical+NIR)
2MASS (JHK)
WISE (4-22 um)
IRAC (3-8 um)
GLIMPSE 360 (3.6-4.5 um)
AKARI color (60-160 um)
PACS color (70-160 um)
SPIRE color (250-500 um)
ATLASGAL (870 um)
ATLASGAL+Planck (870 um)
Bolocam (1.1 mm)
NVSS (1.4 GHz)
Image size
:
arcsec (default is 120 arcsec)
Get selected data
X
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
2MASS K
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.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.freq) as freq FROM oh_data WHERE ref ilike 'LIN91B' 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.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.freq FROM oh_data WHERE ref ilike 'LIN91B' AND detected=true AND hide=false ORDER BY detected DESC,id
