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Acknowledgement
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Data:
OH
BEC92 - A serendipitous survey of the Galactic plane for Type II OH masers
Interferometry data
Short title
: Becker et al. (1992)
Authors
: Becker, Robert H. White, Richard L. Proctor, Deanne D.
Journal
: Astronomical Journal (ISSN 0004-6256), vol. 103, Feb. 1992, p. 544-548.
Bibcode
:
1992AJ....103..544B
Abstract
A 140 deg strip along the Galactic plane with the VLA has been surveyed for OH masers. Fifty OH masers, including 14 new sources, were detected. The masers have a very narrow distribution in Galactic latitude and are probably Population I objects. A study of the IRAS counterparts to OH masers from this and other surveys reveals a strong correlation between the infrared colors of OH masers and Galactic latitude.
Comments:
Spectral type was set to:
""S"", where only one peak was found.
""D"", where two peaks were found.
No velocities are provided.
Sources are OH maser candidates.
Input tables
: Table I
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Table (CSV)
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Detection table from Becker et al. (1992)
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individual components
Detection
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No
Non-detection table from Becker et al. (1992)
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Display associated data
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)
View images
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)
Get selected data
X
Position of H
2
O 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
