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Henize 2-10 is a dwarf starburst galaxy hosting a $\sim10^{6}~M_{\odot}$ black hole (BH) that is driving an ionized outflow and triggering star formation within the central $\sim100$ pc of the galaxy. Here we present ALMA continuum…

星系天体物理 · 物理学 2024-01-08 Hansung B. Gim , Amy E. Reines

Black hole driven outflows have been observed in some dwarf galaxies with active galactic nuclei (1), and likely play a role in heating and expelling gas (thereby suppressing star formation), as they do in larger galaxies (2). The extent to…

星系天体物理 · 物理学 2022-01-24 Zachary Schutte , Amy Reines

Henize 2-10 is a blue dwarf galaxy with intense star formation and one the most intriguing question about it is whether or not it hosts an accretingmassive black hole. We use H and K-band integral field spectra of the inner 130…

星系天体物理 · 物理学 2022-08-19 Rogemar A. Riffel

We present follow-up X-ray observations of the candidate massive black hole (BH) in the nucleus of the low-mass, compact starburst galaxy Henize 2-10. Using new high-resolution observations from the Chandra X-ray Observatory totaling 200 ks…

高能天体物理现象 · 物理学 2016-10-26 Amy Reines , Mark Reynolds , Jon Miller , Gregory Sivakoff , Jenny Greene , Ryan Hickox , Kelsey Johnson

We present single-dish and VLBI observations of an outburst of water maser emission from the young binary system Haro 6-10. Haro 6-10 lies in the Taurus molecular cloud and contains a visible T Tauri star with an infrared companion 1.3"…

太阳与恒星天体物理 · 物理学 2015-06-05 Bruce A. Wilking , Kevin B. Marvel , Mark J. Claussen , Bradley M. Gerling , Alwyn Wootten , Erika Gibb

A candidate accreting massive black hole (BH) with M_BH ~ 10^6 Msun has recently been identified at the center of the dwarf starburst galaxy Henize 2-10 (He 2-10). This discovery offers the first possibility of studying a growing BH in a…

星系天体物理 · 物理学 2015-06-04 Amy E. Reines , Adam T. Deller

We present high spatial resolution mid-IR images of the ring of UCHII regions in W49A obtained at Gemini North, allowing us to identify the driving source of its powerful H2O maser outflow. These data also confirm our previous report that…

太阳与恒星天体物理 · 物理学 2015-05-13 Nathan Smith , Barbara A. Whitney , Peter S. Conti , Chris G. De Pree , James M. Jackson

We report the discovery of H2O maser emission at 1.35 cm wavelength in seven active galactic nuclei (at distances up to <80 Mpc) during a survey conducted at the 70-m diameter antenna of the NASA Deep Space Network near Canberra, Australia.…

We report the detection of water maser emission from four nearby galaxies hosting ultradense HII (UDHII) regions, He 2-10, the Antennae galaxies (NGC 4038/4039), NGC 4214, and NGC 5253, with the Green Bank Telescope. Our detection rate is…

天体物理学 · 物理学 2009-11-13 Jeremy Darling , Crystal Brogan , Kelsey Johnson

We present new ${ }^{12}$CO(J=1-0) observations of Henize 2-10, a blue compact dwarf galaxy about 8.7 Mpc away, taken with the Atacama Large Millimeter Array. These are the highest spatial and spectral resolution observations, to date, of…

星系天体物理 · 物理学 2019-05-29 Nia Imara , Christopher M. Faesi

Observations of H$_2$O masers towards the post-AGB star and water fountain source OH 009.1--0.4 were made as part of HOPS (The H$_2$O southern galactic Plane Survey), with the Mopra radiotelescope. Together with followup observations using…

天体物理学 · 物理学 2008-12-11 A. J. Walsh , S. L. Breen , I. Bains , W. H. T. Vlemmings

We present the results of observations of 22GHz H2O maser emission in NGC 6240 and M51 made with the Karl G. Jansky Very Large Array. Two major H2O maser features and several minor features are detected toward the southern nucleus of NGC…

星系天体物理 · 物理学 2016-02-17 Yoshiaki Hagiwara , Philip G. Edwards

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

Chandra X-ray imaging spectroscopy of the starburst galaxy Henize 2-10 reveals a strong nuclear point source and at least two fainter compact sources embedded within a more luminous diffuse thermal component. Spectral fits to the nuclear…

宇宙学与河外天体物理 · 物理学 2015-05-19 Henry A. Kobulnicky , Crystal L. Martin

Abridged. The LINER galaxy TXS2226-184 is known to host a very luminous 22 GHz water maser, called a gigamaser at the time of its discovery. To date, the nature of this maser is still being debated, in particular, whether it is associated…

星系天体物理 · 物理学 2024-07-29 A. Tarchi , P. Castangia , G. Surcis , V. Impellizzeri , E. Ladu , E. Yu Bannikova

We report dual-frequency very long baseline interferometry (VLBI) observations at 22 and 43 GHz toward the nucleus of a nearby radio galaxy NGC 4261. In particular, we present a VLBI image of the 22 GHz H2O maser line and its location in…

星系天体物理 · 物理学 2023-05-31 Satoko Sawada-Satoh , Nozomu Kawakatu , Kotaro Niinuma , Seiji Kameno

We report the first detection of an extragalactic millimeter wavelength H2O maser at 183 GHz towards NGC 3079 using the Submillimeter Array (SMA), and a tentative submillimeter wave detection of the 439 GHz maser towards the same source…

We report the detection of a 22GHz water maser line in the nearest (D~3.8Mpc) radio galaxy Centaurus A using the Australia Telescope Compact Array (ATCA). The line is centered at a velocity of ~960kms-1, which is redshifted by about…

We present further results of a search for extragalactic submillimeter H2O masers using the Atacama Large Millimeter/Submillimeter Array (ALMA). The detection of a 321 GHz H2O maser in the nearby Type 2 Seyfert galaxy, the Circinus galaxy,…

星系天体物理 · 物理学 2016-08-17 Yoshiaki Hagiwara , Shinji Horiuchi , Akihiro Doi , Makoto Miyoshi , Philip G. Edwards

We report the result of an on-going survey for 22 GHz H2O maser emission towards infrared luminous galaxies. The observed galaxies were selected primarily from the IRAS bright galaxy sample. The survey has resulted in the detection of one…

天体物理学 · 物理学 2009-11-07 Y. Hagiwara , P. J. Diamond , M. Miyoshi
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