On a Transition from Solar-like Coronae to Rotation-dominated Jovian-like Magneto- spheres in Ultracool Main-sequence Stars

Guidelines Abstracts for COOLNEWS are solicited for papers that have been recently accepted by or submitted to refereed journals, and for recent Ph.D. theses. Abstracts for conference proceedings articles are not posted in COOLNEWS. The subject matter should pertain directly to cool stars (spectral types F,G,K,M or L), substellar objects, or the sun. Both theoretical and observational abstracts are appropriate.s for COOLNEWS are solicited for papers that have been recently accepted by or submitted to refereed journals, and for recent Ph.D. theses. Abstracts for conference proceedings articles are not posted in COOLNEWS. The subject matter should pertain directly to cool stars (spectral types F,G,K,M or L), substellar objects, or the sun. Both theoretical and observational abstracts are appropriate. Abstracts dealing with cool pre-main-sequence (PMS) stars will generally not be included in COOLNEWS, since they are already covered by the Star Formation Newsletter. Exceptions to this rule will be considered if the subject matter is truly cross-disciplinary. If you wish to submit a cross-disciplinary abstract on PMS stars, then first submit it to the Star Formation Newsletter. After doing so, submit the abstract to COOLNEWS accompanied by a short e-mail stating that it has already been submitted to the Star Formation Newsletter, and summarizing why it will be of interest to the cool star/solar community at large.s dealing with cool pre-main-sequence (PMS) stars will generally not be included in COOLNEWS, since they are already covered by the Star Formation Newsletter. Exceptions to this rule will be considered if the subject matter is truly cross-disciplinary. If you wish to submit a cross-disciplinary abstract on PMS stars, then first submit it to the Star Formation Newsletter. After doing so, submit the abstract to COOLNEWS accompanied by a short e-mail stating that it has already been submitted to the Star Formation Newsletter, and summarizing why it will be of interest to the cool star/solar community at large. A monthly call for abstracts will be issued and abstracts received by the last day of the month will usually appear in the following month’s newsletter. Announcements of general interest to the cool star and solar communities may also be submitted for posting in the newsletter. These might include (but are not restricted to) the following: (i) Job Openings directed toward cool star or solar researchers, (ii) announcements of Upcoming Meetings, (iii) announcements of Upcoming Observing Campaigns for which participation is solicited from the community at large, (iv) reviews of New Books, and (v) General Announcements that provide or request research-related information. Please send all correspondence to the editor at [email protected]. Abstract templates and back issues can be obtained from the COOLNEWS Web-page at http://casa.colorado.edu/~skinners/coolnews.html . *** Please send abstracts in the body of the message and not as attachments.***