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相关论文: The Egg Nebula (AFGL 2688): Deepening Enigma

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We present the results of B, V, R surface photometry of ESO603-G21 - a galaxy with a possible polar ring. The morphological and photometric features of this galaxy are discussed. The central round object of the galaxy is rather red and…

天体物理学 · 物理学 2009-11-07 V. P. Reshetnikov , M. Faundez-Abans , M. de Oliveira-Abans

We report a multi-wavelength study of two evolved planetary nebulae (PNs) M 2-55 and Abell 2. Deep optical narrow-band images ([O III], H?, and [N II]) of M 2-55 reveal two pairs of bipolar lobes and a new faint arc-like structure. This…

太阳与恒星天体物理 · 物理学 2020-07-29 Chih-Hao Hsia , Yong Zhang , Xi-Liang Zhang , Tao Luo

The curious Galactic features near G357.2$-$0.2 were observed with the MeerKAT radio interferometer array in the UHF and L bands (0.56--1.68 GHz). There are two possibly related features: a newly identified faint heart-shaped partial shell…

高能天体物理现象 · 物理学 2022-08-03 W. D. Cotton , F. Camilo , W. Becker , J. J. Condon , J. Forbrich , I. Heywood , B. Hugo , S. Legodi , T. Mauch , P. Predehl , P. Slane , M. A. Thompson

Extragalactic surveys in the emission line of [O III] 5007 have provided us with the absolute line strengths of large, homogeneous sets of planetary nebulae. These data have been used to address a host of problems, from the measurement of…

宇宙学与河外天体物理 · 物理学 2010-12-28 Robin Ciardullo

We present Herschel Space Observatory photometric observations of the unique, long-period eclipsing binary star Epsilon Aurigae. Its extended spectral energy distribution is consistent with our previously published cool (550 K) dust disk…

星系天体物理 · 物理学 2015-06-04 D. W. Hoard , D. Ladjal , R. E. Stencel , S. B. Howell

We present narrow-band H-alpha, [S II], and [O I] Hubble Space Telescope images of the young planetary nebula GL 618. This object is a compact, bipolar nebula that is currently undergoing the transition from asymptotic giant branch star to…

天体物理学 · 物理学 2009-11-07 Susan R. Trammell , Robert W. Goodrich

CONTEXT: Until now, only one planetary nebula (PN) has been known in the Fornax dwarf spheroidal galaxy. AIMS: The discovery of a second PN candidate, associated with one of the 5 globular clusters in the Fornax dwarf, is reported. METHODS:…

天体物理学 · 物理学 2009-11-13 S. S. Larsen

We present high spectral resolution maps of near-infrared molecular hydrogen emission from the bipolar pre-planetary nebulae RAFGL 2688 and RAFGL 618, obtained with the NOAO Phoenix spectrometer. The measured velocity gradients along the…

天体物理学 · 物理学 2009-10-31 Joel H. Kastner , David A. Weintraub , Ian Gatley , LeeAnn Henn

During our spectroscopic survey of central stars of faint planetary nebulae (PNe), we found that the nucleus of Abell 57 exhibits strong nebular emission lines. Using synthetic narrow-band images, we show that the emission arises from an…

太阳与恒星天体物理 · 物理学 2024-05-21 Howard E. Bond , Akshat S. Chaturvedi , Robin Ciardullo , Klaus Werner , Gregory R. Zeimann , Michael H. Siegel

EGB6 is an extended, faint old planetary nebula (PN) with an enigmatic nucleus. The central star (PG0950+139) is a hot DAOZ-type white dwarf (WD). An unresolved, compact emission knot was discovered to be located 0.166" away from the WD and…

太阳与恒星天体物理 · 物理学 2018-08-29 K. Werner , T. Rauch , J. W. Kruk

Once classified as an emission line source, the planetary nebula (PN) nature of the source Kn 26 has been only recently recognized in digital sky surveys. To investigate the spectral properties and spatio-kinematical structure of Kn 26, we…

星系天体物理 · 物理学 2015-06-12 Martin A. Guerrero , Luis F. Miranda , Gerardo Ramos-Larios , Roberto Vazquez

We present Submillimeter Array (SMA) mapping of $^{12}$CO $J=2\rightarrow 1$, $^{13}$CO $J=2\rightarrow 1$, and CN $N=2\rightarrow 1$ emission from the Ring-like planetary nebula (PN) NGC 3132, one of the subjects of JWST Early Release…

太阳与恒星天体物理 · 物理学 2024-02-21 Joel H. Kastner , David Wilner , Paula Moraga Baez , Jesse Bublitz , Orsola De Marco , Raghvendra Sahai , Al Wootten

The spectra of the planetary nebulae NGC3242 and NGC6369 are reanalysed using spectral measurements made in the mid-infrared with the Spitzer Space Telescope and the Infrared Space Observatory (ISO). The aim is to determine the chemical…

天体物理学 · 物理学 2009-11-13 S. R. Pottasch , J. Bernard-Salas

HH 900 is a peculiar protostellar outflow emerging from a small, tadpole-shaped globule in the Carina nebula. Previous H{\alpha} imaging with HST/ACS showed an ionized outflow with a wide opening angle that is distinct from the highly…

太阳与恒星天体物理 · 物理学 2015-06-23 Megan Reiter , Nathan Smith , Megan M. Kiminki , John Bally , Jay Anderson

In this paper we have analyzed IUE high resolution spectra of the central star (BD+602522) of the Bubble nebula. We discuss velocities of the different regions along the line of sight to the bubble. We find that the Bubble Nebula is younger…

星系天体物理 · 物理学 2009-03-17 M. Y. Anand , B. A. I Kagali , Jayant Murthy

SuWt2 is a planetary nebula (PN) consisting of a bright ionized thin ring seen nearly edge-on. It has a bright (V=12) central star, too cool to ionize the PN, which we discovered to be an eclipsing binary. A spectrum from IUE did not reveal…

太阳与恒星天体物理 · 物理学 2015-05-19 K. Exter , Howard E. Bond , Keivan G. Stassun , B. Smalley , P. F. L. Maxted , D. L. Pollacco

The ionizing star of the planetary nebula NGC 2392 is too cool to explain the high excitation of the nebular shell, and an additional ionizing source is necessary. We use photoionization modeling to estimate the temperature and luminosity…

太阳与恒星天体物理 · 物理学 2012-04-26 Ashkbiz Danehkar , David J. Frew , Quentin A. Parker , Orsola De Marco

We report the discovery of two mid-infrared nebulae in the northern hemisphere with the Wide-field Infrared Survey Explorer and the results of optical spectroscopy of their central stars, BD+60 2668 (composed of two components, separated…

太阳与恒星天体物理 · 物理学 2019-01-30 V. V. Gvaramadze , A. Y. Kniazev , N. Castro , E. K. Grebel

We present narrow-band near-infrared images of a sample of 11 Galactic planetary nebulae (PNe) obtained in the molecular hydrogen (H$_{2}$) 2.122 $\mu$m and Br$\gamma$ 2.166 $\mu$m emission lines and the $K_{\rm c}$ 2.218 $\mu$m continuum.…

太阳与恒星天体物理 · 物理学 2018-06-13 Xuan Fang , Yong Zhang , Sun Kwok , Chih-Hao Hsia , Wayne Chau , Gerardo Ramos-Larios , Martin A. Guerrero

We have conducted a detailed multi-wavelength study of the peculiar nebula Abell 48 and its central star. We classify the nucleus as a helium-rich, hydrogen-deficient star of type [WN4-5]. The evidence for either a massive WN or a low-mass…

太阳与恒星天体物理 · 物理学 2015-12-09 David J. Frew , Ivan S. Bojicic , Q. A. Parker , M. Stupar , S. Wachter , K. DePew , A. Danehkar , M. T. Fitzgerald , D. Douchin