Focal Spot, Fall/Winter 1998

https://digitalcommons.wustl.edu/focal_spot_archives/1080/thumbnail.jp

Spartan Daily, December 7, 2016

Volume 147, Issue 40https://scholarworks.sjsu.edu/spartan_daily_2016/1080/thumbnail.jp

Barnes Hospital Bulletin

https://digitalcommons.wustl.edu/bjc_barnes_bulletin/1080/thumbnail.jp

Spartan Daily, November 20, 2019

Volume 153, Issue 37https://scholarworks.sjsu.edu/spartan_daily_2019/1080/thumbnail.jp

Spartan Daily, November 28, 2017

Volume 149, Issue 39https://scholarworks.sjsu.edu/spartan_daily_2017/1080/thumbnail.jp

Levi Pennington Writing to Mr. Strother, September 2, 1946

Levi Pennington writing to Mr. Strother asking clarifying questions on his status within the Rotary Club.https://digitalcommons.georgefox.edu/levi_pennington/1080/thumbnail.jp

Memorandum on Bargaining Tactics, 1979

Memo to all WCIRA consultants with 102 LRRM 1079-1080 attached discussing Arrow Molded Plastics Inc. and employee participation in illegal and unauthorized work slowdowns

Dense Molecular Gas In A Young Cluster Around MWC 1080 -- Rule Of The Massive Star

We present CS $J = 2 \to 1$, $^{13}$CO $J = 1 \to 0$, and C$^{18}$O $J = 1 \to 0$, observations with the 10-element Berkeley Illinois Maryland Association (BIMA) Array toward the young cluster around the Be star MWC 1080. These observations reveal a biconical outflow cavity with size $\sim$ 0.3 and 0.05 pc for the semimajor and semiminor axis and $\sim$ 45\arcdeg position angle. These transitions trace the dense gas, which is likely the swept-up gas of the outflow cavity, rather than the remaining natal gas or the outflow gas. The gas is clumpy; thirty-two clumps are identified. The identified clumps are approximately gravitationally bound and consistent with a standard isothermal sphere density, which suggests that they are likely collapsing protostellar cores. The gas kinematics suggests that there exists velocity gradients implying effects from the inclination of the cavity and MWC 1080. The kinematics of dense gas has also been affected by either outflows or stellar winds from MWC 1080, and lower-mass clumps are possibly under stronger effects from MWC 1080 than higher-mass clumps. In addition, low-mass cluster members tend to be formed in the denser and more turbulent cores, compared to isolated low-mass star-forming cores. This results from contributions of nearby forming massive stars, such as outflows or stellar winds. Therefore, we conclude that in clusters like the MWC 1080 system, effects from massive stars dominate the star-forming environment in both the kinematics and dynamics of the natal cloud and the formation of low-mass cluster members. This study provides insights into the effects of MWC 1080 on its natal cloud, and suggests a different low-mass star forming environment in clusters compared to isolated star formation.Comment: 42 pages, 5 tables, and 13 figures, accepted for publication in Ap

Letter from an American Supporter in Spain to Geraldine Ferraro

Letter from a American, currently residing in Spain, to Geraldine Ferraro. Author recommends two books, a biography on President Truman and a collection of the Federalist Papers.https://ir.lawnet.fordham.edu/vice_presidential_campaign_correspondence_1984_international/1080/thumbnail.jp