中文
相关论文

相关论文: Multifrequency study of the ring nebula SG13

200 篇论文

We present high resolution radio continuum maps of the Galactic nebula Simeis 57 (= HS 191 = G 80.3+4.7) made with the WSRT and the DRAObservatory at frequencies of 609, 1412 and 1420 MHz. At optical and at radio wavelengths, the nebula has…

天体物理学 · 物理学 2014-10-13 F. P. Israel , M. Kloppenburg , P. E. Dewdney , J. Bally

We present JWST images of the well-known planetary nebula NGC 6720 (the Ring Nebula), covering wavelengths from 1.6$\mu$m to 25 $\mu$m. The bright shell is strongly fragmented with some 20 000 dense globules, bright in H$_2$, with a…

We present sensitive 1-3 GHz ATCA radio continuum observations of the hitherto unresolved star forming region known as either IRAS14482-5857 or PMN1452-5910. At radio continuum frequencies, this source is characterised by a "filled-bubble"…

太阳与恒星天体物理 · 物理学 2015-06-23 D. I. Jones , C. R. Braiding

We present infrared and radio continuum observations of S 201 star forming region. A massive star cluster is observed in this region, which contains different classes of young stellar objects. The near-infrared colour-colour and…

天体物理学 · 物理学 2009-11-10 D. K. Ojha , S. K. Ghosh , V. K. Kulkarni , L. Testi , R. P. Verma , S. Vig

The radio nebula W50 is a unique object interacting with the jets of the microquasar SS433. The SS433/W50 system is a good target for investigating the energy of cosmic-ray particles accelerated by galactic jets. We report observations of…

高能天体物理现象 · 物理学 2021-04-14 Haruka Sakemi , Rikuto Omae , Takumi Ohmura , Mami Machida

Young stellar objects are known to exhibit strong radio variability on timescales of weeks to months, and a few reports have documented extreme radio flares, with at least an order of magnitude change in flux density on timescales of hours…

高能天体物理现象 · 物理学 2017-08-02 Jan Forbrich , Mark J. Reid , Karl M. Menten , Victor Rivilla , Scott J. Wolk , Urvashi Rau , Claire J. Chandler

An investigation in radio and infrared wavelengths of two high-mass star forming regions toward the southern Galactic bubble S10 is presented here. The two regions under study are associated with the broken bubble S10 and Extended Green…

星系天体物理 · 物理学 2016-11-09 Swagat Ranjan Das , Anandmayee Tej , Sarita Vig , Swarna K. Ghosh , Ishwara Chandra C. H.

To observationally explore physical processes, we present a multi-wavelength study of a wide-scale environment toward l = 13.7 - 14.9 degrees containing a mid-infrared bubble N14. The analysis of 12CO, 13CO, and C18O gas at [31.6, 46] km/s…

星系天体物理 · 物理学 2020-07-29 L. K. Dewangan , T. Baug , L. E. Pirogov , D. K. Ojha

We present mid-infrared spectrophotometric observations of SS433 with ISOPHOT. The HeI+HeII lines in both spectra of SS433 and of the Wolf-Rayet star WR147, a wind-colliding WN8+BO5 binary system, closely match. The 2.5-12 micron continuum…

天体物理学 · 物理学 2007-05-23 Yael Fuchs , Lydie Koch-Miramond , Peter Abraham

Context. Abell 1213, a low-richness galaxy system, is known to host an anomalous radio halo detected in data of the VLA. It is an outlier with regard to the relation between the radio halo power and the X-ray luminosity of the parent…

宇宙学与河外天体物理 · 物理学 2023-04-26 W. Boschin , M. Girardi , S. De Grandi , G. Riva , L. Feretti , G. Giovannini , F. Govoni , V. Vacca

This work aims to search for the observational footprints of the interactions between the interstellar medium (ISM) and stellar winds in the Wolf-Rayet (WR) nebula NGC6888 in order to understand its ionization structure, chemical…

NGC 1097 is a nearby SBb galaxy with a Seyfert nucleus and a bright starburst ring. We study the physical properties of the interstellar medium (ISM) in the ring using spatially resolved far-infrared spectral maps of the circumnuclear…

We present APEX observations of CO J=3-2 and ALMA observations of CO J=2-1, 13CO J=2-1 and continuum toward the galactic luminous blue variable AG Car. These new observations reveal the presence of a ring-like molecular structure…

We perform a molecular (CO and CN) line observation using IRAM 30m telescope toward two small regions near the western edge of supernova remnant (SNR) W50/SS433. CO observation reveals spatial correspondence of two molecular clumps at the…

高能天体物理现象 · 物理学 2020-04-21 Qian-Cheng Liu , Yang Chen , Ping Zhou , Xiao Zhang , Bing Jiang

We performed an integral field spectroscopic study for the HII galaxy IIZw70 in order to investigate the interplay between its ionized interstellar medium (ISM) and the massive star formation (SF). Observations were taken in the optical…

天体物理学 · 物理学 2009-11-13 C. Kehrig , J. M. Vilchez , S. F. Sanchez , E. Telles , E. Perez-Montero , D. Martin-Gordon

We present a detailed kinematical analysis of two selected nebulae in the Local Group irregular galaxy IC 1613. The nebulae are: S8, the only known supernova remnant in this galaxy, and S3, a Wolf-Rayet nebula associated with the only WO…

天体物理学 · 物理学 2009-11-06 M. Rosado , M. Valdez-Gutiérrez , L. Georgiev , L. Arias , J. Borissova , R. Kurtev , .

With the aim of studying the properties of Galactic IR bubbles and their impact in massive star formation, we present a study of the IR bubble S169, associated with the massive star forming region IRAS12326-6245. We used…

星系天体物理 · 物理学 2021-02-17 N. U. Duronea , S. Cichowolski , L. Bronfman , E. Mendoza , R. Finger , L. A. Suad , M. Corti , E. M. Reynoso

Messier 15 (NGC 7078) is an old and metal-poor post core-collapse globular cluster which hosts a rich population of variable stars. We report new optical ($gi$) and near-infrared (NIR, $JK_s$) multi-epoch observations for 129 RR Lyrae, 4…

太阳与恒星天体物理 · 物理学 2021-11-24 Anupam Bhardwaj , Marina Rejkuba , G. C. Sloan , Marcella Marconi , Soung-Chul Yang

We present mid-infrared spectra of the microquasar SS 433 obtained with the Infrared Space Observatory (spectroscopic mode of ISOPHOT) and compare them to the spectra of four Wolf-Rayet stars. The mid-infrared spectrum of SS 433 shows…

天体物理学 · 物理学 2007-05-23 Yael Fuchs , L. Koch Miramond , P. Abraham

We discover a large-scale shell G53.9+0.2 around the Crab-like pulsar wind nebula (PWN) G54.1+0.3 with 1420 MHz continuum VLA observations. This is confirmed by a new infrared image at 8 \mu m from the GLIMPSE Legacy Project, which reveals…

天体物理学 · 物理学 2009-11-13 D. A. Leahy , W. W. Tian , Q. D. Wang