Zobrazeno 1 - 10
of 20
pro vyhledávání: '"S. L. Tufte"'
Publikováno v:
The Astrophysical Journal Supplement Series. 149:405-422
The Wisconsin H-Alpha Mapper (WHAM) has surveyed the distribution and kinematics of ionized gas in the Galaxy above declination -30 degrees. The WHAM Northern Sky Survey (WHAM-NSS) has an angular resolution of one degree and provides the first absolu
Publikováno v:
The Astrophysical Journal. 565:1060-1068
We have used the Wisconsin H-Alpha Mapper (WHAM) facility to measure the interstellar H-Alpha emission toward the high Galactic latitude O star HD 93521 (l = 183.1, b = +62.2). Three emission components were detected having radial velocities of -10 k
Publikováno v:
The Astrophysical Journal. 560:L135-L138
We have used the Wisconsin H-Alpha Mapper (WHAM) to observe the spatially extended distribution of ionized hydrogen in M31 beyond the stellar disk. We obtained five sets of observations, centered near the photometric major axis of M31, that extend fr
Publikováno v:
The Astrophysical Journal. 556:L33-L36
The Wisconsin H-Alpha Mapper (WHAM) Northern Sky Survey is revealing that many intermediate-velocity (|v_LSR
12 pages, 3 figures, Figure 1 is full color and a higher quality version will be available on our web site. Published in Astrophysical J
12 pages, 3 figures, Figure 1 is full color and a higher quality version will be available on our web site. Published in Astrophysical J
Autor:
Jeffrey W. Percival, S. M. Nossal, Fred L. Roesler, M. Haffner, Edwin J. Mierkiewicz, J. Bishop, Ronald J. Reynolds, S. L. Tufte
Publikováno v:
Scopus-Elsevier
The Wisconsin Hα Mapper (WHAM), a remotely operable, semi-automated Fabry-Perot located at Kitt Peak Observatory, has been making an all-sky survey of interstellar hydrogen Balmer α(Hα) emissions since 1997. Using the annular summing spectroscopy
Publikováno v:
The Astrophysical Journal. 548:L221-L224
The extremely faint, temperature sensitive ``auroral'' emission line [N II] 5755 has been detected from the low density ionized gas along the sight line toward l = 130.0, b = -7.5 using the Wisconsin H-Alpha Mapper (WHAM). The intensity of this emiss
Publikováno v:
The Astrophysical Journal. 536:335-346
We derive the radio spectral index of the Barnard Loop (BL) from large-scale radio surveys at four frequencies and find it to be a thermal source. We use the radio data together with H-alpha data to determine the electron temperature in BL, the lambd
Publikováno v:
The Astrophysical Journal. 523:223-233
A large portion of the Galaxy (l = 123 deg to 164 deg, b = -6 deg to -35 deg), which samples regions of the Local (Orion) spiral arm and the more distant Perseus arm, has been mapped with the Wisconsin H-Alpha Mapper (WHAM) in the H-Alpha, [S II] 671
Publikováno v:
The Astrophysical Journal. 504:773-784
The first observations of the recently completed Wisconsin H-Alpha Mapper (WHAM) facility include a study of emission lines from high velocity clouds in the M, A, and C complexes, with most of the observations on the M I cloud. We present results inc
Publikováno v:
The Astrophysical Journal. 494:L99-L102
The Wisconsin H? Mapper facility was used to obtain spectra of [O I] ?6300 in three directions that sample the warm ionized component of the interstellar medium at the Galactic midplane and at z-300 pc. Weak interstellar [O I] emission was clearly de