activity
20072022
most citedNuclear ashes and outflow in the eruptive star Nova Vul 1670

60 citations · 134 across the 9 of their papers we have counts for

collaborators

13 papers

astro-ph.SR20226 cited

A search for cool molecular gas in GK Persei and other classical novae

Tomek Kaminski, Helena J. Mazurek, Karl M. Menten +1

Detecting molecular line emission from classical nova remnants has the potential of revealing information on the composition of the ejecta, in particular, it can deliver accurate i…

astro-ph.SR20215 cited

Multiwavelength Observations of the RV Tauri Variable System U Monocerotis: Long-Term Variability Phenomena That Can Be Explained by Binary Interactions with a Circumbinary Disk

Laura D. Vega, Keivan G. Stassun, Rodolfo Montez +7

We present X-ray through submillimeter observations of the classical RV Tauri (RVb-type) variable U Mon, a post-AGB binary with a circumbinary disk (CBD). Our SMA observations indi…

astro-ph.SR2020

Molecular remnant of Nova 1670 (CK Vulpeculae). II. A three-dimensional view on the gas distribution and velocity field

T. Kamiński, W. Steffen, V. Bujarrabal +3

CK Vul is the remnant of an energetic eruption known as Nova 1670 that is thought to be caused by a stellar merger. The remnant is composed of (1) a large hourglass nebula of recom…

astro-ph.SR2020

Molecular remnant of Nova 1670 (CK Vulpeculae): I. Properties and enigmatic origin of the gas

T. Kaminski, K. M. Menten, R. Tylenda +5

CK Vul erupted in 1670 and is considered a stellar-merger candidate. Its remnant contains a molecular component of surprisingly rich composition. We present interferometric line su…

astro-ph.SR202017 cited

SiO maser astrometry of the red transient V838 Monocerotis

Gisela N. Ortiz-Leon, Karl M. Menten, Tomasz Kaminski +3

We present multi-epoch observations with the VLBA of SiO maser emission in the v=1, J=1-0 transition at 43 GHz from the remnant of the red nova V838 Mon. We model the positions of…

astro-ph.SR2019

Cool, evolved stars: results, challenges, and promises for the next decade

Gioia Rau, Rodolfo Montez, Kenneth G. Carpenter +27

Cool, evolved stars are the main source of chemical enrichment of the interstellar medium (ISM), and understanding their mass loss and structure offers a unique opportunity to stud…