Display data from paper

Data:

PAY88 - A young planetary nebula with OH molecules - NGC 6302

Interferometry data

Short title: Payne et al. (1988)
Authors: Payne, H. E. Phillips, J. A. Terzian, Yervant
Journal: Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 326, March 1, 1988, p. 368-375. Research supported by Cornell University.
Bibcode:

Abstract
The results of a sensitive survey of planetary nebulae in all four ground-state OH lines are reported. The results confirm that evolved planetary nebulas are not OH sources in general. However, one interesting object was not detected: an OH 1612 MHz maser in the young planetary nebula NGC 6302. This nebula may be in a brief evolutionary stage, similar to the young and compact planetary nebula Vy 2-2, where OH has already been detected. In addition, the results of further observations of NGC 6302 are reported, including VLA observations of the 1612 MHz line and continuum emission and detections of rotationally excited OH lines at 5-cm wavelength in absorption.

Abstract

The results of a sensitive survey of planetary nebulae in all four ground-state OH lines are reported. The results confirm that evolved planetary nebulas are not OH sources in general. However, one interesting object was not detected: an OH 1612 MHz maser in the young planetary nebula NGC 6302. This nebula may be in a brief evolutionary stage, similar to the young and compact planetary nebula Vy 2-2, where OH has already been detected. In addition, the results of further observations of NGC 6302 are reported, including VLA observations of the 1612 MHz line and continuum emission and detections of rotationally excited OH lines at 5-cm wavelength in absorption.

Input tables: Table 1 and 2
Download as: Table (CSV)
View paper statistics

Detection table from Payne et al. (1988)

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.	Detection
	(J2000)	(J2000)	(deg.)	(deg.)		(MHz)	(km/s)	(km/s)	(km/s)	(km/s)	(Jy)	(Jy)			Yes/No
1	17 13 44.4	-37 06 15.1	349.508004	1.055452	NGC 6302	1667	-54.4	-45.2	-54.4	-45.2	0.090	0.11	ENG15	PAY88	-H₂O +OH
2	19 24 21.8	+09 53 55.7	45.497178	-2.70183	VY 2-2	1612	-62.0		-62.0		4.640		ENG15	PAY88	-H₂O +OH
3	17 13 44.4	-37 06 15.1	349.508004	1.055452	NGC 6302	1612	-51.3	-40.5	-51.3	-40.5	0.140	0.55	ENG15	PAY88	-H₂O +OH

Non-detection table from Payne et al. (1988)

Export table to csv

Hide / Show individual components

Detection
Yes/No

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)
			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

Display data from paper

PAY88 - A young planetary nebula with OH molecules - NGC 6302

Interferometry data

View paper statistics

Detection table from Payne et al. (1988)

Non-detection table from Payne et al. (1988)