Fig. 8 from SiO Maser Survey of the Galactic Disk IRAS Sources. II. |l| ≤ 3° and |b| ≤ 3°, the Galactic Center Area

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SiO Maser Survey of the Galactic Disk IRAS Sources. II. |l| ≤ 3° and |b| ≤ 3°, the Galactic Center Area

Authors: Shuji Deguchi, Takahiro Fujii, Hideyuki Izumiura, Osamu Kameya, Yoshikazu Nakada, Jun-ichi Nakashima, Takafumi Ootsubo, and Nobuharu Ukita

SiO Maser Survey of Galactic Disk IRAS Sources. II. 2000 The Astrophysical Journal Supplement Series 128 571.

Provider: AAS Journals

Caption: Fig. 8.

Longitude–velocity diagram of the doubly peaked OH 1612 MHz sources (Sevenster et al. 1997). The filled and unfilled circles indicate the sources in the central nuclear disk (﹩\vert l\vert < ﹩1° and ﹩\vert b\vert < ﹩﹩0\fdg 5﹩ in Fig. 7) and elsewhere, respectively. Least‐squares fits are shown for the nuclear disk sources (broken line) and all the OH 1612 MHz sources in ﹩\vert l\vert < 3﹩° and ﹩\vert b\vert < 3﹩° (thin line).

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