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相关论文: ATCA observations of SiO masers in the Galactic ce…

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The infrared dark cloud G359.94+0.17 is a conspicuous, opaque cloud, which is seen in silhouette against the Galactic center. We found unexpectedly strong (~50 Jy) maser emission of CH3OH at 44 GHz with additional weak 22 GHz H2O maser and…

星系天体物理 · 物理学 2015-05-30 S. Deguchi , D. Tafoya , N. Shino

We report here on multi-frequency VLBA observations of three extragalactic sources within 1 degree of the Galactic Center. These sources have been used as astrometric reference sources for VLA and VLBA determinations of the proper motion of…

天体物理学 · 物理学 2016-08-30 Geoffrey C. Bower , Donald C. Backer , Richard A. Sramek

Context. The compact radio and near-infrared (NIR) source Sagittarius A* (Sgr A*) associated with the supermassive black hole in the Galactic center was observed at 7 mm in the context of a NIR triggered global Very Long Baseline Array…

星系天体物理 · 物理学 2016-02-17 C. Rauch , E. Ros , T. P. Krichbaum , A. Eckart , J. A. Zensus , B. Shahzamanian , K. Muzic

(Abridged) In this paper, we investigate the physical conditions of [CI]-traced gas in high-mass star-forming regions by analyzing APEX [CI] 492 GHz single-pointing observations of the ATLASGAL Top100 sources along with other…

星系天体物理 · 物理学 2022-08-17 Min-Young Lee , Friedrich Wyrowski , Karl Menten , Maitraiyee Tiwari , Rolf Guesten

We present radio and infrared observations indicating on-going star formation activity inside the $\sim2-5$ pc circumnuclear ring at the Galactic center. Collectively these measurements suggest a continued disk-based mode of on-going star…

Discovered in 1995 at the Caltech Submillimeter Observatory (CSO), the vibrationally-excited water maser line at 658 GHz (455 micron) is seen in oxygen-rich giant and supergiant stars. Because this maser can be so strong (up to thousands of…

天体物理学 · 物理学 2015-03-30 T. R. Hunter , K. H. Young , R. D. Christensen , M. A. Gurwell

A survey of young bipolar outflows in regions of low-to-intermediate-mass star formation has been carried out in two class I methanol maser transitions: 7_0-6_1A+ at 44 GHz and 4_{-1}-3_0E at 36 GHz. We detected narrow features towards NGC…

星系天体物理 · 物理学 2015-05-18 S. V. Kalenskii , L. E. B. Johansson , P. Bergman , S. Kurtz , P. Hofner , C. M. Walmsley , V. I. Slysh

We report the detection of a new H2CO maser in the massive star forming region G23.71-0.20 (IRAS 18324-0820), i.e., the fifth region in the Galaxy where H2CO maser emission has been found. The new H2CO maser is located toward a compact HII…

天体物理学 · 物理学 2009-11-11 E. Araya , P. Hofner , W. M. Goss , S. Kurtz , H. Linz , L. Olmi

We present 44 and 226 GHz observations of the Galactic center within 20$"$ of Sgr A*. Millimeter continuum emission at 226 GHz is detected from eight stars that have previously been identified at near-IR and radio wavelengths. We also…

高能天体物理现象 · 物理学 2017-08-02 F. Yusef-Zadeh , R. Schödel , M. Wardle , H. Bushouse , W. Cotton , M. J. Royster , D. Kunneriath , D. A. Roberts , E. Gallego-Cano

Despite their carbon-rich photospheres, silicate carbon stars show evidence of oxygen-rich circumstellar material, which is considered to exist in disks. Silicate carbon stars represent interesting cases that allow us to study the possible…

太阳与恒星天体物理 · 物理学 2013-10-18 K. Ohnaka , D. A. Boboltz , G. Mulitz-Schimel , H. Izumiura , M. Wittkowski

We report here BIMA array observations of linear polarization in Sagittarius A*, the compact radio source in the Galactic Center. These observations had a resolution of 20 arcsec x 5 arcsec oriented North-South. We do not detect linear or…

天体物理学 · 物理学 2009-11-06 Geoffrey C. Bower , Melvyn C. H. Wright , Heino Falcke , Donald C. Backer

We report on the detection of SiO masers in Asymptotic Giant Branch variables toward bulge/disk globular clusters. In five out of six cases, the radial velocities are compatible with the optically measured radial velocities of globular…

天体物理学 · 物理学 2015-06-24 Noriyuki Matsunaga , Shuji Deguchi , Yoshifusa Ita , Toshihiko Tanabe , Yoshikazu Nakada

We present 321 GHz observations of five AGN from ALMA Cycle 0 archival data: NGC 5793, NGC 1068, NGC 1386, NGC 4945, and the Circinus galaxy. Submillimeter maser emission is detected for the first time towards NGC 4945, and we present a new…

星系天体物理 · 物理学 2016-08-17 D. W. Pesce , J. A. Braatz , C. M. V. Impellizzeri

The central region of the Galaxy has been observed at 580, 620 and 1010 MHz with the Giant Metrewave Radio Telescope (GMRT). We detect emission from Sgr-A*, the compact object at the dynamical centre of the Galaxy, and estimate its flux…

天体物理学 · 物理学 2009-11-10 Subhashis Roy , A. Pramesh Rao

We have used the Australia Telescope Compact Array (ATCA) to conduct further observations of the 36.2-GHz ($4_{-1}\rightarrow3_0$E) methanol transition towards the nearby active galaxy NGC 4945. These observations have led to a more…

星系天体物理 · 物理学 2018-08-22 Tiege P. McCarthy , Simon P. Ellingsen , Shari L. Breen , Christian Henkel , Maxim A. Voronkov

We present results of our Chandra observation with the ACIS-I instrument centered on the position of Sagittarius A* (Sgr A*), the compact nonthermal radio source associated with the massive black hole (MBH) at the dynamical center of the…

A new methanol maser line 6(-1)-5(0)E at 133 GHz was detected with the 12-m Kitt Peak radio telescope using remote observation mode from Moscow. Moderately strong, narrow maser lines were found in DR21(OH), DR21-W, OMC-2, M8E, NGC2264,…

天体物理学 · 物理学 2009-10-30 V. I. Slysh , S. V. Kalenskii , I. E. Val'tts , V. V. Golubev

We present high-resolution Karl G. Jansky Very Large Array observations of the 22 GHz $\mathrm{H_2O}$ maser line in the extended Sagittarius B2 cloud. We detect 499 $\mathrm{H_2O}$ masers across the observed velocities between -39 and 172…

Observations of dust-enshrouded evolved stars selected from infrared catalogs requiring high positional accuracy, like infrared spectroscopy or long baseline radio interferometric observations, often require preparational observational…

We report on the first 1,432 sources observed using the Atacama Large Millimeter/submillimeter Array (ALMA), from the Bulge Asymmetries and Dynamical Evolution (BAaDE) survey, which aims to obtain tens of thousands of line-of-sight…