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相关论文: Theory and Extragalactic Masers

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We have used the Australia Telescope Compact Array (ATCA) to search for 6.7-GHz methanol maser emission towards 87 galaxies. We chose the target sources using several criteria, including far-IR luminosities and the presence of known OH…

天体物理学 · 物理学 2020-11-25 C. J. Phillips , R. P. Norris , S. P. Ellingsen , D. P. Rayner

Investigations of H$_2$O maser galaxies at X-ray energies reveal that most AGN associated with water masers are characterized by high levels of absorption. With the aim of finding new maser sources for possible interferometric follow-ups,…

星系天体物理 · 物理学 2019-09-04 P. Castangia , G. Surcis , A. Tarchi , A. Caccianiga , P. Severgnini , R. Della Ceca

Extragalactic water vapor masers with 50, 1000, 1, and 230 solar (isotropic) luminosities were detected toward Mrk1066 (UGC2456), Mrk34, NGC3556 and Arp299, respectively. The interacting system Arp299 appears to show two maser hotspots…

天体物理学 · 物理学 2009-11-10 C. Henkel , A. B. Peck , A. Tarchi , N. M. Nagar , J. A. Braatz , P. Castangia , L. Moscadelli

We discuss the region of transition between galactic and extragalactic cosmic rays. The exact shapes and compositions of these two components contains information about important parameters of powerful astrophysical sources and the…

天体物理学 · 物理学 2008-11-26 Todor Stanev

In the early days of methanol maser discoveries the 9(2)-10(1) A+ transition at 23.1 GHz was found to exhibit maser characteristics in the northern star-forming region W3(OH), and probable maser emission in two other sources. Attention…

天体物理学 · 物理学 2009-11-10 D. M. Cragg , A. M. Sobolev , J. L. Caswell , S. P. Ellingsen , P. D. Godfrey

NGC6240 is a well-studied nearby galaxy system in the process of merging. Based on optical, X-ray, and radio observations, it is thought to harbor two active nuclei We carried out a detailed optical 3D spectroscopic study to investigate the…

星系天体物理 · 物理学 2020-01-15 W. Kollatschny , P. M. Weilbacher , M. W. Ochmann , D. Chelouche , A. Monreal-Ibero , R. Bacon , T. Contini

We present results from a deep (1 sigma = 5.7 mJy beam^{-1} per 20.8 km s^{-1} velocity channel) ^{12}CO(1-0) interferometric observation of the central 60" region of the nearby edge-on starburst galaxy NGC 2146 observed with the Nobeyama…

The understanding of the nature of ultra-high-energy cosmic rays is one of the most intriguing open questions for current and future observatories. These particles are expected to be accelerated in extragalactic sources. Because of their…

高能天体物理现象 · 物理学 2016-12-28 Mariangela Settimo

The first VLBI images of water maser emission in the Circinus Galaxy AGN show both an accretion disk and outflow 0.1 to 1 pc from the central engine. The maser traces a warped, edge-on accretion disk between radii of about 0.1 and 0.4 pc…

天体物理学 · 物理学 2007-05-23 L. J. Greenhill

We present the results of second epoch ALMA observations of 321 GHz H$_2$O emission toward two nearby active galactic nuclei, NGC 4945 and the Circinus galaxy, together with Tidbinbilla 70-m monitoring of their 22 GHz H$_2$O masers. The two…

星系天体物理 · 物理学 2022-01-05 Yoshiaki Hagiwara , Shinji Horiuchi , Masatoshi Imanishi , Philip G. Edwards

High precision mapping of H2O megamaser emission from active galaxies has revealed more than a dozen Keplerian H2O maser disks, which enable a ~4% uncertainty estimate of the Hubble constant as well as providing accurate masses for the…

22 GHz water vapor `kilomaser' emission is reported from the central region of the Whirlpool galaxy M 51 (NGC 5194). The red-shifted spectral features (Vlsr ~ 560 km/s), flaring during most of the year 2000, originate from a spatially…

天体物理学 · 物理学 2016-08-30 Yoshiaki Hagiwara , Christian Henkel , Karl. M. Menten , Naomasa Nakai

We discuss Hubble Space Telescope optical images and spectra of NGC 6251, a giant E2 galaxy and powerful radio source at a distance of 106 Mpc (for H_0 = 70 km/s/Mpc). The galaxy is known to host a very well defined dust disk (O'Neil et al.…

天体物理学 · 物理学 2009-10-31 Laura Ferrarese , Holland Ford

As part of the Megamaser Cosmology Project (MCP), here we present a new geometric distance measurement to the megamaser galaxy NGC 5765b. Through a series of VLBI observations, we have confirmed the water masers trace a thin, sub-parsec…

星系天体物理 · 物理学 2016-02-03 F. Gao , J. A. Braatz , M. J. Reid , K. Y. Lo , J. J. Condon , C. Henkel , C. Y. Kuo , C. M. V. Impellizzeri , D. W. Pesce , W. Zhao

We report VLA 1 sigma upper limits of 1.5% and 3% on the intrinsic circular and linear fractional polarizations, respectively, of the water vapor maser emission 0.2 pc from the central engine of NGC 4258. A corresponding 0.5% upper limit on…

天体物理学 · 物理学 2009-10-30 J. R. Herrnstein , J. M. Moran , L. J. Greenhill , E. G. Blackman , P. J. Diamond

We have used the Australia Telescope Compact Array (ATCA) to observe the 36.2-GHz class I methanol maser emission towards NGC253 and find that it is located at the interface between the nuclear ring and both ends of the galactic bar. This…

星系天体物理 · 物理学 2017-09-20 Simon Ellingsen , Xi Chen , Shari Breen , Hai-Hua Qiao

A multi-line millimeter-wave study of the nearby starburst galaxy NGC 4945 has been carried out using the Swedish-ESO Submillimeter Telescope (SEST). The study covers the frequency range from 82 GHz to 354 GHz and includes 80 transitions of…

天体物理学 · 物理学 2009-11-10 M. Wang , C. Henkel , Y. -N. Chin , J. Whiteoak , M. Cunningham , R. Mauersberger , D. Muders

We present the results of the first dedicated survey for 22 GHz H$_2$O maser emission in dwarf galaxies outside of the local group, with the aim of discovering disc masers. Studies of disc masers yield accurate and precise measurements of…

星系天体物理 · 物理学 2020-10-21 M. J. Rosenthal , I. Zaw

Methanol masers at 6.7~GHz are well-known signposts of high-mass star-forming regions. [...] We aim to understand the origin of the ring-like structures outlined by methanol maser emission in a number of sources. This emission could be, a…

星系天体物理 · 物理学 2024-06-19 A. Bartkiewicz , A. Sanna , M. Szymczak , L. Moscadelli , H. J. van Langevelde , P. Wolak , A. Kobak , M. Durjasz

We argue that if ultrahigh-energy (E > 10^10 GeV) cosmic rays are heavy nuclei (as indicated by existing data), then the pointing of cosmic rays to their nearest extragalactic sources is expected for 10^10.6 < E/GeV < 10^11. This is because…

高能天体物理现象 · 物理学 2017-12-25 Luis A. Anchordoqui , Vernon Barger , Thomas J. Weiler
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