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相关论文: H$_2$ Emission Nebulosity Associated with KH 15D

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Far ultraviolet emission has been detected from a knot of Halpha emission in the Horseshoe filament, far out in the NGC 1275 nebula. The flux detected relative to the brightness of the Halpha line in the same spatial region is very close to…

宇宙学与河外天体物理 · 物理学 2015-06-05 R. M. Johnstone , R. E. A. Canning , A. C. Fabian , G. J. Ferland , M. Lykins , R. L. Porter , P. A. M. van Hoof , R. J. R. Williams

The unique eclipsing, weak-lined T Tauri star KH 15D has been detected as an X-ray source in a 95.7 ks exposure from the Chandra X-ray Observatory archives. A maximum X-ray luminosity of 1.5 x 10^{29} erg s$^{-1}$ is derived in the 0.5--8…

天体物理学 · 物理学 2009-11-11 William Herbst , Edward C. Moran

We report infrared spectroscopy of the unusual eclipsing pre-main sequence object KH 15D, obtained using NIRSPEC on Keck II. During eclipse, observations using low spectral resolution (1000) reveal the presence of prominent molecular…

天体物理学 · 物理学 2009-11-10 Drake Deming , David Charbonneau , Joseph Harrington

We present near-IR narrow-band continuum-subtracted images in the H$_2$ $2.122\mu$m, and Br$\gamma$ $2.166\mu$m emission lines for a sample of 15 bipolar planetary nebulae. H$_2$ emission was definitely detected for most of the objects in…

天体物理学 · 物理学 2009-10-31 M. A. Guerrero , E. Villaver , A. Manchado , P. Garcia-Lario , F. Prada

Integral-field spectroscopy of molecular hydrogen in the optical wavelength region and complementary long-slit near-infrared spectroscopy are presented towards HH91A.The detection of some 200 H_2 lines arising from ro-vibrational levels up…

天体物理学 · 物理学 2009-11-13 Roland Gredel

KH 15D is a well-known spectroscopic binary because of its unique and dramatic photometric variability. The variability is explained by a circumbinary dust ring but the ring itself was never directly detected. We present a new…

太阳与恒星天体物理 · 物理学 2019-07-10 Min Fang , Ilaria Pascucci , Jinyoung Serena Kim , Suzan Edwards

Emission from the $2_{12}-1_{11}$ line of H$_2$CO has been detected and marginally resolved toward LkCa15 by the Nobeyama Millimeter Array. The column density of H$_2$CO is higher than that observed in DM Tau and than predicted by…

We present infrared echelle spectroscopy of three Herbig-Haro (HH) driving sources (SVS 13, B5-IRS 1 and HH 34 IRS) using Subaru-IRCS. The large diameter of the telescope and wide spectral coverage of the spectrograph allowed us to detect…

天体物理学 · 物理学 2009-11-13 M. Takami , A. Chrysostomou , T. P. Ray , C. J. Davis , W. R. F. Dent , J. Bailey , M. Tamura , H. Terada , T. S. Pyo

We report the detection of quiescent H2 emission in a spatially resolved ring-like structure within 100 AU of T Tau N. We present evidence to show that the emission most likely arises from shocks in the atmosphere of a nearly face-on disk…

天体物理学 · 物理学 2009-11-13 M. Gustafsson , L. Labadie , T. M. Herbst , M. Kasper

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 present near-infrared spectroscopy of fluorescent molecular hydrogen (H_2) emission from molecular filaments in the reflection nebula NGC 7023. We derive the relative column densities of H_2 rotational-vibrational states from the…

天体物理学 · 物理学 2009-10-30 Paul Martini , K. Sellgren , Joseph L. Hora

We present VRIJHK photometry of the KH 15D T Tauri binary system for the 2015/16 and 2016/17 observing seasons. For the first time in the modern (CCD) era we are seeing Star B fully emerge from behind the trailing edge of the precessing…

太阳与恒星天体物理 · 物理学 2018-01-10 Rachel A. Aronow , William Herbst , A. Meredith Hughes , David J. Wilner , Joshua N. Winn

This paper reports detections of H$\alpha$ emission and stellar continuum out to approximately 30 physical kpc, and H$\alpha$ directionality in the outskirts of H$\alpha$-emitting galaxies (H$\alpha$ emitters) at $z=0.4$. This research…

星系天体物理 · 物理学 2022-02-23 Rhythm Shimakawa , Masayuki Tanaka , Satoshi Kikuta , Masao Hayashi

We present detailed geometry and kinematics of the inner outflow toward HL Tau observed using Near Infrared Integral Field Spectograph (NIFS) at the Gemini-North 8-m Observatory. We analyzed H2 2.122 um emission and [Fe II] 1.644 um line…

天体物理学 · 物理学 2009-11-13 Michihiro Takami , Tracy L. Beck , Tae-Soo Pyo , Peter McGregor , Christopher Davis

We perform a multi-wavelength study of a two-ribbon flare on 2002 September 29 and its associated filament eruption, observed simultaneously in the H-alpha line by a ground-based imaging spectrograph and in hard X-rays by RHESSI. The flare…

天体物理学 · 物理学 2009-11-10 M. D. Ding , Q. R. Chen , J. P. Li , P. F. Chen

Deep optical CCD images of the supernova remnant G 15.1-1.6 were obtained and filamentary and diffuse emission has been discovered. The images, taken in the emission lines of Halpha+[N II], [S II] and [O III], reveal filamentary and diffuse…

天体物理学 · 物理学 2009-11-13 P. Boumis , J. Alikakos , P. E. Christopoulou , F. Mavromatakis , E. M. Xilouris , C. D. Goudis

Near-infrared Fabry-Perot imaging has revealed H2 emission extended to about 130 pc from the disk of NGC 253. It is closely related to the hot plasma observed in soft X-rays: filamentary H2 features are found at the edges of the hot plasma.…

天体物理学 · 物理学 2009-11-07 H. Sugai , R. I. Davies , M. J. Ward

We detect near-infrared H2 emission in DG Tau using the Infrared Camera and Spectrograph (IRCS) on the 8.2-m SUBARU telescope. The spectra obtained along the jet axis show that the centroidal position of the 1-0 S(1) emission is offset by…

天体物理学 · 物理学 2009-11-10 M. Takami , A. Chrysostomou , T. P. Ray , C. Davis , W. R. F. Dent , J. Bailey , M. Tamura , H. Terada

We present K-band integral field observations of the circumstellar envelope of the evolved star OH 231.8+4.2. Spatial and spectral information were simultaneously acquired using the Sinfoni integral field unit, with adaptive optics, on the…

太阳与恒星天体物理 · 物理学 2015-06-03 K. P. Forde , T. M. Gledhill

A simple analytic model is presented to predict the near-IR H2 fluorescent line intensities emitted by diffuse interstellar clouds with a Plummer density profile. It is applicable to sightlines where (1) the column densities of H and H2…

星系天体物理 · 物理学 2024-10-15 David A. Neufeld
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