A large high velocity cloud at lII = 41°, bII = −15°
نویسندگان
چکیده
منابع مشابه
Deep H i observations of the compact high - velocity cloud HVC 125 + 41 – 207
We present deep H i observations of the compact high-velocity cloud HVC125+41–207 using the 100m Effelsberg telescope. Our goal was in particular to study the warm neutral medium (WNM) in detail. The Effelsberg data reveals a two phase core/halo structure – one component with a velocity width of FWHM ≈ 5 km s (Westerbork data show FWHM ≈ 2 km s, Braun & Burton 2000) and one with FWHM ≈ 18 km s....
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By comparing sensitive Spitzer Space Telescope (SST) infrared and Green Bank Telescope 21 cm observations, we are able to report the first detection of dust emission in Complex C, the largest High Velocity Cloud in the sky. Dust in the region of Complex C studied here has a colder temperature (T = 10.7 −0.8 K 1σ) than the local interstellar medium (T = 17.5 K), in accordance with its great dist...
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In the spectra of 139 early-type Large Magellanic Cloud (LMC) stars observed with FUSE and with deep radio Parkes H I 21-cm observations along those stars, we search for and analyze the absorption and emission from high-velocity gas at +90 ≤ vLSR ≤ +175 km s . The H I column density of the high-velocity clouds (HVCs) along these sightlines ranges from < 10 to 10 cm. The incidence of the HVC met...
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We present the results of CO J = 2 → 1 observations of the X-ray bright giant shell complex 30 Doradus in the Large Magellanic Cloud (LMC) using the Antarctic Submillimeter Telescope and Remote Observatory (AST/RO). This is the one of the largest H II complexes in the Local Group. We compare the CO J = 2 → 1 observations against previously taken CO J = 4 → 3 observations and analyze the spatial...
متن کاملIRAC Observations of CO J = 4 → 3 High - Velocity Cloud in the 30 Doradus Complex in the Large Magellanic Cloud
We present the results of CO J = 2 → 1 observations of the X-ray bright giant shell complex 30 Doradus in the Large Magellanic Cloud (LMC) using the Antarctic Submillimeter Telescope and Remote Observatory (AST/RO). This is the one of the largest H II complexes in the Local Group. We compare the CO J = 2 → 1 observations against previously taken CO J = 4 → 3 observations and analyze the spatial...
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ژورنال
عنوان ژورنال: Symposium - International Astronomical Union
سال: 1964
ISSN: 0074-1809
DOI: 10.1017/s0074180900052426