Allen Lawrence, wrapping up a long career as an electrical engineer, was serious about moving his astronomy hobby beyond the 20-inch telescope he’d hauled to star parties under the dark skies of Texas and Arizona.
So in 2011 – in his late 60s, after 30 years of operating his own consulting firm around Green Bay, Wisconsin – he enrolled in some courses at the University of Wisconsin-Madison. It wasn’t long before he went around Sterling Hall asking about joining a research team.
Jay Gallagher, now the W. W. Morgan & Rupple Bascom Emeritus Professor of Astronomy at Wisconsin, offered Lawrence the chance to study one of two galaxy systems. Lawrence picked a nearby system studied since the 1960s and featuring the interaction of two galaxies, a larger one known as NGC 4490 (nicknamed the “Cocoon Galaxy” because of its shape) and a smaller one known as NGC 4485. The system is about 20% the size of the Milky Way, located in the Northern Hemisphere and about 30 million light years from Earth.
After taking a look at some infrared images from NASA’s Wide-field Infrared Survey Explorer, Lawrence said it looked like the larger galaxy had a rare double nucleus. One nucleus could be seen in visible wavelengths, the other nucleus was hidden in dust and could only be seen in infrared and radio wavelengths.
Well – after years of study, including earning an Iowa State University master’s degree in 2018 and continuing to work with Iowa State astronomers – Lawrence, at 77, is the first author of a paper revealing the NGC 4490 galaxy does, indeed, have a double nucleus. The paper is now online and has been accepted for publication by the Astrophysical Journal.
Co-authors of the paper are Iowa State’s Charles Kerton, an associate professor of physics and astronomy; and Curtis Struck, a professor of physics and astronomy; as well as East Tennessee State University’s Beverly Smith, a professor of physics and astronomy.
“I saw the double nucleus about seven years ago,” Lawrence said. “It had never been observed – or nobody had ever done anything with it before.”
Some astronomers may have seen one nucleus with their optical telescopes. And others may have seen the other with their radio telescopes. But he said the two groups never compared notes to observe and describe the double nucleus.
The new paper describes “a clear double nucleus structure.” It says both nuclei are similar in size, mass and luminosity. It says both are similar in mass and luminosity to the nuclei observed in other interacting galaxy pairs. And, it says the double nucleus structure could also explain why the galaxy system is surrounded by an enormous plume of hydrogen.
“The most straightforward interpretation of the observations is that NGC 4490 is itself a late-stage merger remnant” of a much-earlier collision of two galaxies, the authors wrote. A merger could drive and extend the high level of star formation necessary to create such a large hydrogen plume.
The astronomers said there are other reasons they find the study of this system interesting:
Struck, who studies colliding galaxies, said double-nucleus galaxies are very rare, especially in smaller galaxies such as this one. And, he said astronomers think a double nucleus could contribute to the buildup of super massive black holes found in the center of some galaxies.
And Kerton, who researches star formation, said, “This project demonstrates that using multiple wavelengths from space- and ground-based observations together can really help us understand a particular object.”
Reference: “Revealing the Double Nucleus of NGC 4490” by AL Lawrence, C. R. Kerton, Curtis Struck, Beverly J. Smith, 16 January 2020, Astrophysics of Galaxies.